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	<title>radiation &#8211; Fountain Magazine</title>
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		<title>FLASH Radiotherapy</title>
		<link>https://fountainmagazine.com/all-issues/2021/issue-140-mar-apr-2021/flash-radiotherapy/</link>
		
		<dc:creator><![CDATA[Louima Cunningham]]></dc:creator>
		<pubDate>Mon, 01 Mar 2021 12:31:57 +0000</pubDate>
				<category><![CDATA[Issue 140 (Mar - Apr 2021)]]></category>
		<category><![CDATA[medicine]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[technology]]></category>
		<category><![CDATA[therapy]]></category>
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					<description><![CDATA[FLASH radiotherapy is a brand-new model of radiation therapy that may be administered to a cancer patient in as little as a single, complete treatment. The therapy lasts much less than one second and has a duration of up to six weeks. Comparatively, conventional radiation therapy takes several minutes to administer the same dose. Introduction [&#8230;]]]></description>
										<content:encoded><![CDATA[<p><img fetchpriority="high" decoding="async" class=" size-full wp-image-7071" src="https://fountainmagazine.com/wp-content/uploads/2021/03/02-b42.jpg" alt="FLASH Radiotherapy" width="1920" height="1200" srcset="https://fountainmagazine.com/wp-content/uploads/2021/03/02-b42.jpg 1920w, https://fountainmagazine.com/wp-content/uploads/2021/03/02-b42-300x188.jpg 300w, https://fountainmagazine.com/wp-content/uploads/2021/03/02-b42-1024x640.jpg 1024w, https://fountainmagazine.com/wp-content/uploads/2021/03/02-b42-768x480.jpg 768w, https://fountainmagazine.com/wp-content/uploads/2021/03/02-b42-1536x960.jpg 1536w" sizes="(max-width: 1920px) 100vw, 1920px" /></p>
<p>FLASH radiotherapy is a brand-new model of radiation therapy that may be administered to a cancer patient in as little as a single, complete treatment. The therapy lasts much less than one second and has a duration of up to six weeks. Comparatively, conventional radiation therapy takes several minutes to administer the same dose.</p>
<h2>Introduction</h2>
<p>Radiotherapy is one of the predominant scientific remedies for tumors. The goals of radiotherapy are twofold; the first of which lies in successfully killing tumor cells with ionizing radiation, and the second is, at the same time, minimizing regular tissue damage that negatively influences the affected person&#8217;s care and quality of life. It is estimated that up to 65% of tumor patients go through radiotherapy at one point during their treatment. The first thing to do to reach these goals is to deposit a high amount of powerful ionizing radiation onto a tumor while at the same time avoiding irradiating regular tissue. Recent decades have seen a rise of new, superior technology consisting of intensity-modulated radiotherapy, stereotactic body radiotherapy, proton, and carbon particle radiotherapy. These new devices and techniques have converted radiotherapy into a particular and effective therapy routine for most cancer sufferers with the aid of using enhanced spatial dose administration. Nevertheless, the therapy of radiation-resistant tumors continues to be confined with the aid of using dose-proscribing regular tissue complications.</p>
<p>The second thing to do to achieve successful radiation is to grow the differential reaction among regular tissue and tumors to ionize radiation with the aid of using, for instance, a hyper-fractionated therapy strategy. Conventional radiotherapy (CONV-RT) contains fractions of two Gy (or “gray”; a measurement used for radiation) per day for five days (Monday to Friday) every week for numerous weeks, permitting regular tissues to get over radiation-precipitated damaging results to an extra quantity than tumors, whose radiation reaction is dictated with the aid of using the whole dose introduced as opposed to with the aid of using the dose given at every fraction. Recently, a third method to for precise aiming, known as FLASH-RT, emerged as a promising new device in presenting temporal administration of a single dose of high dose rate ionizing radiation.</p>
<h2>What is new in Radiation Therapy?</h2>
<p>Conventional RT has developed significantly over time. However, the harm precipitated to healthy tissues at some point of the radiation therapy continues to be a vital task for traditional RT.</p>
<p>FLASH RT represents an entire archetypal shift as opposed to an improvement upon the present era of radiotherapy technology. The variety of research is continuously growing to an accumulation of promising outcomes. FLASH RT is perhaps one of the most promising technologies for tumor therapy, imparting vital views for preclinical studies.</p>
<h2>Advantages of Flash radiation therapy compared to conventional radiation therapy</h2>
<p>FLASH RT complements the differential impact among tumors and healthy tissues. FLASH RT provides doses in an extraordinarily brief irradiation time as a quick “flash” of radiation. FLASH RT is iso-powerful whilst in comparison to standard dose rate RT, thus decreasing regular tissue toxicity and side effects.</p>
<p>Conventional radiotherapy (RT) is significantly confined by radiation-precipitated toxicities. If those could be decreased, an extra dose of radiation might be given thus facilitating a higher tumor reaction.</p>
<p>The ultra-speedy administration of radiation therapy (i.e., electrons, photons/x-rays, and protons) at dose rates numerous orders-of-importance extra than the ones presently utilized in scientific exercise reduces radiation-precipitated toxicities. This permits regular tissue tolerance stages to be substantially exceeded, thereby growing the healing index over traditional radiation administration.</p>
<p>In traditional external beam radiotherapy (EBRT), the affected person is irradiated for 1-2 minutes, 5-days/wk, for 1-2 months. In FLASH-RT, the affected person might be irradiated in &lt; 0.1 second for 1 to four days thus substantially decreasing side-effects, regular tissue toxicity, and cost.</p>
<h2>Tissue toxicity</h2>
<p>It was first discovered in the 1960’s that non-cancerous cells that were subjected to ultra-high dose rates of radiotherapy had been much more likely to be viable than the ones subjected to standard dose rates. This has been currently supported with the aid of using research in mice, and was validated that there was much less harm in the lungs of mice treated with FLASH-RT in comparison to the ones treated with CONV-RT. In every other examination, mice subjected to complete brain irradiation at traditional dose rates were worse in recognition checks in comparison to the ones treated at ultra-high dose rates. Radiation-precipitated pores and skin reactions can encompass reddening and breakdown and have been proven to be greatly decreased in rodents being treated with FLASH-RT in comparison to CONV-RT. FLASH-RT additionally compared favorably in a single examine evaluating the pores and skin response of a mini-pig to distinctive dose rates of radiotherapy. Another examination related to the therapy of nasal cancers in cats with FLASH-RT confirmed the entire remission of tumors with minimum trauma to surrounding tissues. Researching the FLASH impact is of importance to set up how it could be utilized in a scientific situation to deal with most cancer patients.</p>
<p>Many research studies show that further to decreasing tissue toxicity, FLASH-RT additionally produces an identical tumor reaction as CONV-RT.</p>
<h2>Influencing elements</h2>
<p>There is an array of elements that could have an effect on the efficacy of FLASH treatment which includes dose rate, general dose, pulse rate, fractionation, and modality of radiation. The dose rate used for the FLASH impact may additionally range relying upon the affected tissue and the administration approach. Many studies vary in the general dose of radiation used, or use doses inconceivable in scientific scenarios, which complicate the findings. The supply of radiation is likewise an aspect because FLASH impact has been primarily discovered by using electron linear accelerators. More currently, the success of FLASH treatment has additionally been visible following usage of proton and X-ray radiation. Pulsing the radiation at a high frequency can result in FLASH therapy at an appropriate dose-in line with-pulse. Furthermore, the examination is wanted to verify the important parameters for inducing the FLASH impact, as there are a wide variety of variables at work.</p>
<h2>Oxygen depletion</h2>
<p>Exactly why the FLASH impact happens is not absolutely understood but has been hypothesized. Hypoxic tissues (tissues which might be disadvantaged of oxygen) are greatly immune to radiation (and are consequently much less likely to be damaged) than well-oxygenated tissues. It is therefore conceptualized that the distinction in tissue toxicity among FLASH-RT and CONV-RT can be because of the extent of hypoxia at ultra-high dose rates and ensuing radioresistance transferred to irradiated tissue.</p>
<h2>Changes in immunity</h2>
<p>Another proposed idea for FLASH treatment to have a greater impact is a changed immune reaction. Since it utilizes a shorter therapy time, much fewer lymphocytes (white blood cells concerned within the immune gadget) suffer from the radiation. One examination mentioned much less immune gadget activation in mice following FLASH-RT in comparison to CONV-RT. It has to be referred to that it&#8217;s far doubtful if any immune reaction following FLASH-RT is contributing to the FLASH impact or because of it. Other organic responses consisting of DNA harm and infection can also be contributing, and greater research is needed for clarification.</p>
<h2>Conclusion</h2>
<p>FLASH-RT provides a single burst of high dosage rate ionizing radiation in milliseconds and achieves near perfect tumor control and, at the same time, spares regular tissues from extreme aspect results. The result is the presentation of fascinating imaginative and prescient of enhancing scientific results for tumor sufferers with the aid of using the use of dose-rate modulation of radiotherapy. The FLASH impact gives advanced tissue safety in comparison to CONV-RT without compromising on tumor therapy. It has been studied throughout numerous species and now a single human case has been documented. While its mechanism of motion is likely to contain oxygen depletion, it isn&#8217;t always absolutely understood and consequently calls for similar examination. The doses required to acquire the FLASH impact make it unsuitable for many patient studies. Furthermore, the provision of radiation sources to generating appropriate beams for the therapy of each superficial and deep tumor is a proscribing aspect in scientific trials. If future studies yield greater know-how of the organic mechanisms of the FLASH impact, it will be viable to acquire it at decreased doses, growing its scientific viability.</p>
<h2>References</h2>
<ol>
<li>https://www.mdpi.com/1422-0067/21/18/6492</li>
<li>Jonathan R. Hughes and Jason L. Parsons.: “FLASH Radiotherapy: Current Knowledge and Future Insights Using Proton-Beam Therapy”. Int. J. Mol. Sci. 2020, 21(18), 6492; Cancer Research Centre, Department of Molecular and Clinical Cancer Medicine, University of Liverpool, 200 London Road, Liverpool L3 9TA, UK And  Clatterbridge Cancer Centre NHS Foundation Trust, Clatterbridge Road, Bebington CH63 4JY, UK.</li>
<li>https://www.sciencedirect.com/science/article/pii/S26665557203000833 4. Guangming Zhou. : Mechanisms underlying FLASH radiotherapy, a novel way to enlarge the differential responses to ionizing radiation between normal and tumor tissues. Radiation Medicine and Protection. Volume 1, Issue 1, March 2020, Pages 35-40</li>
<li>https://isensors.net/flash-rt/5.</li>
<li>https://researchoutreach.org/articles/flash-radiotherapy-what-how-why/#:</li>
<li>J. D. Wilson, E. M. Hammond, G. S. Higgins, K. Petersson (2020) Ultra-High Dose Rate (FLASH) Radiotherapy: Silver Bullet or Fool’s Gold? Frontiers in Oncology 9, 1563.</li>
</ol>
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		<title>Our Skin and Protection from the Sun</title>
		<link>https://fountainmagazine.com/all-issues/2019/issue-130-july-aug-2019/our-skin-and-protection-from-the-sun/</link>
		
		<dc:creator><![CDATA[The Fountain]]></dc:creator>
		<pubDate>Mon, 01 Jul 2019 23:26:55 +0000</pubDate>
				<category><![CDATA[Issue 130 (July - Aug 2019)]]></category>
		<category><![CDATA[body]]></category>
		<category><![CDATA[damage]]></category>
		<category><![CDATA[effects]]></category>
		<category><![CDATA[health]]></category>
		<category><![CDATA[layer]]></category>
		<category><![CDATA[light]]></category>
		<category><![CDATA[melanoma]]></category>
		<category><![CDATA[minutes]]></category>
		<category><![CDATA[people]]></category>
		<category><![CDATA[person]]></category>
		<category><![CDATA[protection]]></category>
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		<category><![CDATA[rays]]></category>
		<category><![CDATA[Science]]></category>
		<category><![CDATA[skin]]></category>
		<category><![CDATA[solar]]></category>
		<category><![CDATA[spf]]></category>
		<category><![CDATA[sun]]></category>
		<category><![CDATA[type]]></category>
		<category><![CDATA[uva]]></category>
		<category><![CDATA[uvb]]></category>
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					<description><![CDATA[Enveloping our body like a piece of clothing, our skin is a miraculous organ that both forms a barrier against potential invaders and plays a crucial role in the maintenance of vital functions. It is a mirror that reflects our experiences, memories, and fate with the lines and marks on it. With a surface area [&#8230;]]]></description>
										<content:encoded><![CDATA[<p><img decoding="async" class=" size-full wp-image-6727" src="https://fountainmagazine.com/wp-content/uploads/2019/07/09_Skin_B-466.jpg" alt="Our Skin and Protection from the Sun" width="900" height="1142" srcset="https://fountainmagazine.com/wp-content/uploads/2019/07/09_Skin_B-466.jpg 900w, https://fountainmagazine.com/wp-content/uploads/2019/07/09_Skin_B-466-236x300.jpg 236w, https://fountainmagazine.com/wp-content/uploads/2019/07/09_Skin_B-466-807x1024.jpg 807w, https://fountainmagazine.com/wp-content/uploads/2019/07/09_Skin_B-466-768x975.jpg 768w" sizes="(max-width: 900px) 100vw, 900px" /></p>
<p>Enveloping our body like a piece of clothing, our skin is a miraculous organ that both forms a barrier against potential invaders and plays a crucial role in the maintenance of vital functions. It is a mirror that reflects our experiences, memories, and fate with the lines and marks on it. With a surface area of 1.72 square meters and a weight of approximately 9.6 kg, including the fatty tissue under it, the skin is the largest organ in our body and life cannot possibly be maintained without it.<a href="#_edn1" name="_ednref1">[1]</a> It is through the skin that we learn knives cut, fire burns, and our mother has very soft hands. We don’t even realize, but the skin quietly carries out other numerous functions such as sweating toxins out of the body, maintaining body temperature, and synthesizing vitamin D.<a href="#_edn2" name="_ednref2">[2]</a> Some of these functions are related to the sun and the protection of our body from it.</p>
<p>The sun emits all kinds of rays across the electromagnetic spectrum. The lethal ones among these rays are filtered by the atmosphere that envelops the Earth, so very few of these dangerous rays reach the land.<a href="#_edn3" name="_ednref3">[3]</a> The rays that reach Earth are visible (wavelengths of 400-700 nm) and ultraviolet (wavelengths of 100-400 nm) rays. Ultraviolet radiation comes in three types: UVA, UVB, and UVC.</p>
<p>Having wavelengths of 320-400 nm, UVA rays make up 90% of the UV that reaches Earth’s surface. Regardless of whether it is cloudy or sunny, the same amount of these rays reaches Earth and penetrates as far as the lower layers of the human skin. UVA rays damage the connective tissue under the skin, causing the skin to get old and the formation of free radicals, which indirectly cause DNA damage, hence terminal skin cancers or melanoma. Rays that come in these wavelengths are also largely responsible for allergic reactions on the skin.</p>
<p>With wavelengths of 280-320 nm, UVB rays make up 5-10% of the UV radiation reaching Earth. These rays help with the synthesis of vitamin D but also cause sunburns and the synthesis of melanin in the skin. UVB rays also have a role in mutating genes that prevent growth of tumors, thus leading to the development of skin cancers other than melanoma.</p>
<p>With wavelengths of 100-280 nm, UVC rays are harmful to living things. When they reach the Earth’s atmosphere, UVC rays interact with the oxygen atoms here. This interaction leads to the formation of the ozone layer, which prevents UVC rays from almost never reaching the ground. These dangerous waves have been put into humankind’s service by being employed in the creation of the protective ozone layer.</p>
<h3>Ultraviolet rays and the harmful effects of visible light on the skin</h3>
<p>There are short-term and long-term effects of UV rays on the skin.</p>
<p>The short-term effects are sunburn, heat stroke, allergic reactions, suntan, and viral diseases such as herpes, which are usually felt shortly after exposure to the sun and can be triggered by suppression of the immune system. The long-term, accumulative effects are photo-aging (the skin getting wrinkly due to solar rays), sunspots, cataracts, and the development of skin cancers.<a href="#_edn4" name="_ednref4">[4]</a></p>
<p>On the other hand, our skin is not entirely unprotected against the dangerous effects of the sun. The keratin layer in the epidermis, the uppermost layer of the skin, absorbs or disperses light, so the amount of light penetrating into the layers below is significantly lowered. Beta-carotene in the skin along with some enzyme systems reduce free oxygen radicals released after exposure to the sun and thus eliminate solar damage. Likewise, melanin, which gives our skin its color, lies above the nuclei in skin cells and acts as an umbrella that protects the cellular DNA from solar radiation.<a href="#_edn5" name="_ednref5">[5]</a></p>
<p>Six subgroups of skin types have been determined according to color of the hair, eyes, and skin, as well as the skin’s reaction to solar rays. This classification is widely accepted for identifying risk groups and determining specific protection measures.<a href="#_edn6" name="_ednref6">[6]</a></p>
<p>Although the number of melanosomes, or melanin-producing cells in the human skin, is the same in all humans, the color of the skin is determined by the genetic differences in the type, amount, and size of melanin pigments. Melonosomes in Europeans are small and light, while those of Africans are larger and darker.<a href="#_edn7" name="_ednref7">[7]</a></p>
<h3>The importance of protection from the sun</h3>
<p>The frequency of skin cancer has been increasing, which is precipitated by the fact that the ozone layer has gotten thinner and people are not well informed about UV protection. Many people take beach vacations and sunbathe, do mountain sports, have tanned skin, work in open air professions (such as construction workers, lifeguards, and tour guides), and they do so without much care.</p>
<p>For protection, we should first know that harmful effects of solar rays accumulate over time. The damage caused by the sun is stored in the body, just like change we save in a piggy bank. Unfortunately, we accumulate 40-50% of the total damage we are exposed to in a lifetime in the first quarter of life – that is, during childhood and our teenage years.<a href="#_edn8" name="_ednref8">[8]</a> The skin’s natural protection mechanisms are not fully developed during these periods, nor is our understanding of protection. A research study carried out in Australia has shown that the rate of malign melanoma seen in young people can be reduced by 73% through effective solar protection methods.<a href="#_edn9" name="_ednref9">[9]</a></p>
<p>The major reason for wrinkles, the primary and fundamental indication of aging skin, is not in fact our age but the sun. UVA and UVB rays break down the connective tissue below the skin, disrupt the skin’s repair mechanisms, and cause skin aging (or photo-aging). Therefore, photo-aging takes place faster and earlier in people who work outside.<a href="#_edn10" name="_ednref10">[10]</a></p>
<p>{Picture: Photo-aging visible on one side of a truck driver’s face}<a href="#_edn11" name="_ednref11">[11]</a> </p>
<p>It’s imperative that we begin teaching children and adolescents about UV protection: having suffered five sunburns in childhood and early youth increases the risk of developing melanoma by 80%.<a href="#_edn12" name="_ednref12">[12]</a> Children shouldn’t spend long hours in the midday, summer sun. </p>
<p>Solar damage isn’t just more likely in children and teenagers, but also in people with skin type 1 or 2 (light skin), red hair, and/or colored eyes (blue); people, especially light-skinned people, with many skin moles; people whose family members have or had skin cancer; those who have a skin disorder triggered by the sun (lupus, dermatomyositis, rosacea); and people who have innate light sensitivity (albino, xeroderma pigmentosum, etc.). All these groups must be particularly careful about protecting themselves from the sun.</p>
<p>What are some ways to protect ourselves from UV Rays? Well, because UV radiation bombards the Earth most intensely at noon during the summer, staying indoors is greatly recommended between the hours of 10:00 am and 4:00 pm.  Additionally, the reflection rate of solar rays is higher by the seaside and in snowy environments.<a href="#_edn13" name="_ednref13">[13]</a></p>
<p>Wearing appropriate clothes is still the most effective and the least expensive method of sun protection. Clothing can have a solar protection factor (SPF) of 15-30. The level of protection is determined by the type of fabric, number of pores, and type, color, and thickness of weaving. The best clothes are made from cotton, silk, and denim and are unbleached and woven tightly. Wet clothes are more permeable. The use of wide hats, sunglasses, and umbrellas are also important for protection.</p>
<p>In addition to these measures, sun protection creams should also be used. The idea that protection creams will prevent the synthesis of vitamin D, voiced frequently lately, should not prevent the use of sun protection because the solar rays we receive during the day from the face and hands are sufficient for the synthesis of vitamin D. A person should pick a sun cream appropriate for their skin and apply it in sufficient amounts 20 minutes before going out. Babies should be protected through natural means, and physical sun protection should be used for children and pregnant women. A person should reapply sun protection products every two or three hours while outside, and, if planning to swim, they should choose water resistant products.</p>
<p>Besides physical protection that blocks, scatters, or reflects solar rays, there are also skin-absorbable chemical protections with cosmetically accepted formulations that eliminate light by absorbing it.</p>
<p>Generally speaking, a good sun protection should protect against both UVA and UVB rays. It should be cosmetically acceptable, non-toxic, water and perspiration resistant, and at the appropriate SPF (sun protection factor) level. However, because reapplication is required every two to three hours, protection above SPF 50 is the same. Therefore, it is no use buying a more expensive, higher protection product.<a href="#_edn14" name="_ednref14">[14]</a> For people with type 3 skin (darker white skin with gold tone), SPF 30 is sufficient. For light skinned people, children, and pregnant women, however, SPF 50 is recommended.</p>
<p>SPF is the number indicating by how many more times a sunscreen protects the skin against UVB than the skin itself. Skin type is very important in sunscreen choice. The natural protection period of a person with type 1 skin is 5-10 minutes, while it may go up to 90 minutes for a person with type 6 skin. In other words, a light-skinned person gets a sunburn in 5-10 minutes of exposure, while a dark-skinned person may not get one at all. Therefore, these people should not choose products at the same SPF level. For example, if the skin’s self-protection duration is five minutes, a sunscreen with a SPF of 30 provides the same protection for 150 minutes.</p>
<p>Apart from sun protection creams, oral products can also help with sun protection. For example, oral zinc intake is proven to prevent cellular and DNA damage caused by UV radiation. Vitamin C is effective at preventing UVA rays due to its antioxidant properties and vitamin E at preventing UVB rays. In addition, the intake of beta carotene (a precursor of vitamin A) and bioflavonoids (also called vitamin P which generally has effects similar to vitamin C), found in orange and red fruit, protects against UV damage. Polyphenolic compounds in green tea also display protective properties against UV radiation.<a href="#_edn15" name="_ednref15">[15]</a></p>
<p>Finally, we should remember that using a sun protection product is a small part of our attitude toward your overall protection from the sun. Considering the role of the ozone layer in filtering the sun’s harmful rays, we should protect the perfect balance in the universe and re-evaluate our responsibilities and future actions for the maintenance of this balance.</p>
<h3>Notes</h3>
<p><a href="#_ednref1" name="_edn1">[1]</a> livescience.com.</p>
<p><a href="#_ednref2" name="_edn2">[2]</a> Gilchrest BA. “Sun exposure and vitamin D sufficiency,” <em>Am. J Clin Nutr</em>. August 2008, Vol. 88 # 2 570S-577S.</p>
<p><a href="#_ednref3" name="_edn3">[3]</a> Understanding UVA and UVB. skincancer.org.</p>
<p><a href="#_ednref4" name="_edn4">[4]</a> sciencelearn.org.nz.</p>
<p><a href="#_ednref5" name="_edn5">[5]</a> “The Protective Role of Melanin against UV Damage in Human Skin.” <em>Photochem Photobiol</em>. 2008; 84(3):539-549.</p>
<p><a href="#_ednref6" name="_edn6">[6]</a> laserdocs.co.uk/easy-way-to-find-out-your-fitzpatrick-skin-type/</p>
<p><a href="#_ednref7" name="_edn7">[7]</a> Ibid.</p>
<p><a href="#_ednref8" name="_edn8">[8]</a> Adele CG, Sarah C Wallingford and Penelope M. “Childhood exposure to UV radiation and harmful skin effects: Epidemiological evidence.” <em>Prog Biophys Mol Biol</em>. December 2011, 107(3): 349-355.</p>
<p><a href="#_ednref9" name="_edn9">[9]</a> Green AC, Williams GC, Logan V, Srutton GM. “Reduced Melanoma after Regular Sunscreen Use: Randomized Trial Follow-Up,” <em>Journal of Clinically Oncology</em>. 20 January 2011, Vol. 29 # 3:257-263.</p>
<p><a href="#_ednref10" name="_edn10">[10]</a> Fitzpatrick’s Dermatology in General Medicine.</p>
<p><a href="#_ednref11" name="_edn11">[11]</a> www.nejm.org/doi/full/10.1056/NEJMicm1104059.</p>
<p><a href="#_ednref12" name="_edn12">[12]</a> Markovic SN, Erickson LA, Rao RD, et al. “Malignant Melanoma in the 21<sup>st</sup> Century, part 1: Epidemiology, risk factors screening, prevention and diagnosis.” <em>Mayo Clin Proc</em>, 2007; 82: 364-380.</p>
<p><a href="#_ednref13" name="_edn13">[13]</a> Skin cancer prevention and early detection. www.skincancer.org.</p>
<p><a href="#_ednref14" name="_edn14">[14]</a> www.dermnetz.org.</p>
<p><a href="#_ednref15" name="_edn15">[15]</a> Halliwell B. “Free radicals, antioxidants and human disease.” Lancet 1994; 344-:721-724.</p>
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		<title>Beware: Radiation!</title>
		<link>https://fountainmagazine.com/all-issues/2018/issue-126-november-december-2018/beware-radiation/</link>
		
		<dc:creator><![CDATA[Nuh Yilmaz]]></dc:creator>
		<pubDate>Thu, 01 Nov 2018 20:21:06 +0000</pubDate>
				<category><![CDATA[Issue 126 (Nov - Dec 2018)]]></category>
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		<category><![CDATA[devices]]></category>
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		<category><![CDATA[sar]]></category>
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					<description><![CDATA[Radiation, which refers to emissions of light or particles, is a type of energy transfer. Radiation takes place at any given moment in the environment or the body. Among sources of radiation to which humans are exposed daily are sun rays, radio waves coming from devices such as mobile phones and TV sets, appliances such [&#8230;]]]></description>
										<content:encoded><![CDATA[<p><img decoding="async" class=" size-full wp-image-6626" src="https://fountainmagazine.com/wp-content/uploads/2018/11/52-519.jpg" alt="Beware: Radiation!" width="1920" height="1200" srcset="https://fountainmagazine.com/wp-content/uploads/2018/11/52-519.jpg 1920w, https://fountainmagazine.com/wp-content/uploads/2018/11/52-519-300x188.jpg 300w, https://fountainmagazine.com/wp-content/uploads/2018/11/52-519-1024x640.jpg 1024w, https://fountainmagazine.com/wp-content/uploads/2018/11/52-519-768x480.jpg 768w, https://fountainmagazine.com/wp-content/uploads/2018/11/52-519-1536x960.jpg 1536w" sizes="(max-width: 1920px) 100vw, 1920px" /></p>
<p>Radiation, which refers to emissions of light or particles, is a type of energy transfer. Radiation takes place at any given moment in the environment or the body. Among sources of radiation to which humans are exposed daily are sun rays, radio waves coming from devices such as mobile phones and TV sets, appliances such as ovens or irons that emit heat, and medical machines such as ultrasounds. The radiation emitted from devices and machines do not cause ionization. Ionizing radiation is made up of high-energy wavelengths or particles, and this is the kind of radiation we get from x-ray, CT, and nuclear imaging. This is used to penetrate tissue to reveal the body’s internal organs and structures. Ionizing radiation can damage DNA, and when our cells cannot fully repair the damage, this may result in DNA mutations.<a href="#_ftn1" name="_ftnref1">[1]</a> The radiation which poses real danger to humans and has the power to ionize is when radioactive—or unstable—atoms decay and emit alpha (α), beta (β), and gamma (γ) rays.</p>
<p>The earth, air, water, and all living things are more or less radioactive because radioactive atoms are everywhere. The average person is annually exposed to radiation levels of 2.6 – 10 mSv (millisievert), which is not that alarming. The maximum limit recommended for people exposed to radiation for occupational reasons is 100 mSv. The lungs of a person who smokes one pack of cigarettes a day are exposed to an annual radiation of 106 mSv.</p>
<p><span id="more-5440"></span></p>
<h3><strong>How can we protect ourselves?</strong></h3>
<p>It is recommended by the World Health Organization that children younger than 16 should not use mobile phones; when they do, their calls should not exceed 10 minutes. When purchasing devices, you should also take into account its SAR (Specific Absorption Rate). Prefer devices with a SAR&lt;1 W/kg. It is also recommended to unplug electrical devices when you are not using them, to keep electrical appliances as far away from your head as possible, use the hairdryer for short periods and in intervals, and to avoid using mobile phones for long conversations (or use headphones!).</p>
<p>It’s also worth reconsidering whether using radiation-emitting devices such as mammography, x-rays, or ultrasounds are absolutely necessary. In 2010, the British Department of Health and Social Care banned using tomography for screening purposes. Another study in the US found that one in ten people are exposed to high levels of radiation because of medical tests.</p>
<p>The average radiation rates (mSv) a person was exposed to during use of certain imaging devices is as follows:</p>
<table>
<tbody>
<tr>
<td width="88">
<p>Full Body Tomography</p>
</td>
<td width="88">
<p>Colonoscopy</p>
</td>
<td width="85">
<p>Head</p>
<p>Tomography</p>
</td>
<td width="80">
<p>Mammography</p>
</td>
<td width="77">
<p>Chest Ultrasound</p>
</td>
<td width="77">
<p>Tooth</p>
<p>X-Ray</p>
</td>
<td width="77">
<p>Arm</p>
<p>X-Ray</p>
</td>
</tr>
<tr>
<td width="88">
<p>10</p>
</td>
<td width="88">
<p>10</p>
</td>
<td width="85">
<p>2</p>
</td>
<td width="80">
<p>0.4</p>
</td>
<td width="77">
<p>0.1</p>
</td>
<td width="77">
<p>0.01</p>
</td>
<td width="77">
<p>0.001</p>
</td>
</tr>
</tbody>
</table>
<p>Researchers also found that employees in nuclear power plants were exposed to amounts of radiation that far exceeded allowable amounts.</p>
<h3><strong>Beware of radon</strong></h3>
<p>The natural radiation humans are exposed to most is the gas radon. Some matter with radioactive atoms such as uranium and thorium – both present in the earth since its birth – emit radon, which seeps through the earth and into the walls of houses and through gaps in plumbing. It is recommended to air houses at least 15 minutes every 24 hours as the only way to be protected from radon.</p>
<h3><strong>The resistance of living things</strong></h3>
<p>Creatures have been created with different forms of resistance to the elements, including radiation. For example, dogs have a lower resistance than humans, while many other creatures such as rabbits, tortoises, and fruit flies have a higher resistance. And then there is the cockroach, which can survive even a nuclear attack. The lethal radiation dose for cockroaches is an incredible 670- 1000 Sv, whereas it is 6-8 Sv for humans.</p>
<p>Scorpions are also much more radiation-resistant than humans. They can withstand up to 1500 Sv, an amount that is 250 times the maximum dose humans can take. Studies have found a correlation between the strength of a scorpion’s venom and their resistance to radiation. The greater the amount of venom, the greater the resistance they have. The presence of the neural transmitter serotonin supports this view.</p>
<h3><strong>Are humans radioactive too?</strong></h3>
<p>Humans contain trace amounts of radioactive atoms, namely uranium (<sup>238</sup>U), potassium (<sup>40</sup>K), and carbon (<sup>14</sup>C). An 80 kg human has natural radiation of 8000 becquerel every second, which is equal to 100Bq per kilogram. This amount is not high enough to cause any worry. The human body has 40 trillion cells on average, and every cell has about 100 trillion atoms. The proportion of the radiating atoms in the body is about 8000/4&#215;10<sup>21</sup>.</p>
<h3><strong>Precision protection</strong></h3>
<p>The radioactive atoms in the body with the highest probability for carcinogenic effects are potassium (<sup>40</sup>K) and carbon (<sup>14</sup>C) atoms. The decomposition that leads to cancer stems from mutations in genes, but the molecules that are the building blocks of genes do not have potassium atoms. The likelihood that a cell gets harmed is very low: it is necessary that the particles emitted from the radioactive potassium atom crash into the DNA molecule and harm it, which is as unlikely as threading a needle when blindfolded. The DNA is precisely protected inside the nucleus located at the center of the cell. If we consider the fact that the average diameter of a cell is about 10 microns (1 micron is one-thousandth of a millimeter), we can better appreciate how little space DNA occupies.</p>
<p>Radiocarbon atoms (<sup>14</sup>C), on the other hand, might be present in DNA molecules, and they are more dangerous because the emitted particles are more likely to find the target despite having weaker radioactive properties than potassium. A radioactive carbon atom turns into a nitrogen (<sup>14</sup>N) atom and may thus cause a chemical change in the DNA. In other words, the carbon atom is possibly to blame for the unexpected development of cancer.</p>
<p>The likelihood of harmful radioactive particles hitting a person’s DNA is low, and the protective system provided for it lowers the likelihood of developing cancer even more. New DNA molecules that form during DNA coupling are repeatedly checked by inspector enzymes. If there is an error, it is detected and then corrected. The broken code is taken out to be replaced with the correct version. Meanwhile, all these steps are checked by other enzymes assigned to the task. More errors might be made in the newly produced DNA molecule because of external factors. Yet ribosomes in the cell start to produce repair enzymes, as per the instructions from the DNA.</p>
<p>When thinking about all the protective factors that have been coded into the DNA for our survival against the 8000 radioactive activities that occur in our body every second, one cannot help but feel awe for the infinite mercy and wisdom that operate in our lives.</p>
<h3><strong>References</strong></h3>
<ul>
<li>http://time.com/5069317/california-mobile-phone-radiation/</li>
<li>https://www.health.harvard.edu/cancer/radiation-risk-from-medical-imaging</li>
<li>Choppin, G. et al., <em>Radiochemistry and Nuclear Chemistry</em>, Oxford: Elsevier Science &amp; Technology, 1995.</li>
<li>www.physics.isu.edu/radinf/natural.htm</li>
</ul>
<p><a href="#_ftnref1" name="_ftn1">[1]</a> https://www.health.harvard.edu/cancer/radiation-risk-from-medical-imaging</p>
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		<title>How Do Animals Survive?</title>
		<link>https://fountainmagazine.com/all-issues/2018/issue-126-november-december-2018/how-do-animals-survive/</link>
		
		<dc:creator><![CDATA[Numan Erciyes]]></dc:creator>
		<pubDate>Thu, 01 Nov 2018 14:11:26 +0000</pubDate>
				<category><![CDATA[Issue 126 (Nov - Dec 2018)]]></category>
		<category><![CDATA[animals]]></category>
		<category><![CDATA[Antifreeze]]></category>
		<category><![CDATA[chemical]]></category>
		<category><![CDATA[clay]]></category>
		<category><![CDATA[creature]]></category>
		<category><![CDATA[dolphins]]></category>
		<category><![CDATA[expert]]></category>
		<category><![CDATA[find]]></category>
		<category><![CDATA[humans]]></category>
		<category><![CDATA[live]]></category>
		<category><![CDATA[living]]></category>
		<category><![CDATA[lungs]]></category>
		<category><![CDATA[macaw]]></category>
		<category><![CDATA[oxygen]]></category>
		<category><![CDATA[plants]]></category>
		<category><![CDATA[protect]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[Science]]></category>
		<category><![CDATA[scientists]]></category>
		<category><![CDATA[species]]></category>
		<category><![CDATA[substance]]></category>
		<category><![CDATA[survive]]></category>
		<category><![CDATA[Tardigrades]]></category>
		<category><![CDATA[water]]></category>
		<category><![CDATA[Zoology]]></category>
		<guid isPermaLink="false">http://107.21.79.195/all-issues/2018/issue-126-november-december-2018/how-do-animals-survive/</guid>

					<description><![CDATA[We live in a magnificent world inhabited by approximately 8,700,000 species. This number includes only general species, not subspecies. Scientists discover around 2,500 new species every year, and the number is soon estimated to reach 10 million. All living organisms are blessed with unique bodies, systems, and organs, defense and protection mechanisms to survive and [&#8230;]]]></description>
										<content:encoded><![CDATA[<p><img loading="lazy" decoding="async" class=" size-full wp-image-6618" src="https://fountainmagazine.com/wp-content/uploads/2018/11/29-2-371.jpg" alt="How Do Animals Survive?" width="1920" height="1200" srcset="https://fountainmagazine.com/wp-content/uploads/2018/11/29-2-371.jpg 1920w, https://fountainmagazine.com/wp-content/uploads/2018/11/29-2-371-300x188.jpg 300w, https://fountainmagazine.com/wp-content/uploads/2018/11/29-2-371-1024x640.jpg 1024w, https://fountainmagazine.com/wp-content/uploads/2018/11/29-2-371-768x480.jpg 768w, https://fountainmagazine.com/wp-content/uploads/2018/11/29-2-371-1536x960.jpg 1536w" sizes="auto, (max-width: 1920px) 100vw, 1920px" /></p>
<p>We live in a magnificent world inhabited by approximately 8,700,000 species. This number includes only general species, not subspecies. Scientists discover around 2,500 new species every year, and the number is soon estimated to reach 10 million.</p>
<p>All living organisms are blessed with unique bodies, systems, and organs, defense and protection mechanisms to survive and protect themselves, and special features to help them forage for food.</p>
<p><span id="more-5432"></span></p>
<p>When people get ill due to environmental effects or malnutrition they usually consult a doctor. They try to find a cure by using the medicine prescribed by doctors. However, animals living in the wild don’t have this option. When animals living in nature or on the street get ill what can they do if nobody takes them to a vet? How do millions of species get well and find cures for their ailments?</p>
<p>You might think that animals who become sick in the wild must simply live with their symptoms, but this is not the case. In fact, we have given a clue at the introduction: each organism is equipped with features to lead a self-sustaining life. Either their bodily functions perfectly enable them to live in their habitat or their unique metabolisms protect them from harmful external factors. Animals also can use some plants whose health benefits have only recently been discovered by humans.</p>
<p>In recent decades, there has been a growing interest for herbal products such as walnut leaf, cherry stalk tangerine rind, grenadine red, and celery root to find cure for diseases.</p>
<blockquote>
<p>Animals perform amazing tasks with mind-blowing adroitness as if each were an expert chemist. Wondrous mechanisms are activated when a need arises to protect animals from harm.</p>
</blockquote>
<h3><strong>Some plants with healing properties: </strong></h3>
<p>Lupine, quassia, bitter wood, hemlock, fishberry, roselle, henbane, giant fennel root, pistachio, resin, pine turpentine, mistletoe, cumin, hibiscus, hibiscus flower, alkanet, flos elaeagni, camphor, cardamom, St John&#8217;s wort, French lavender, Flaxseed, linseed oil, henna tree, quillaia, wall germander, cranberry, aspand, daffodil, water lily, common balm and eucalyptus.</p>
<p>Animals have been consuming and finding cures in these plants since the dawn of time. They are also equipped with many surviving capabilities under extremely severe conditions. Here are a few examples:</p>
<h3><strong>Antibiotics expert</strong></h3>
<p>With a height of up to five meters, the giraffe is the tallest land animal. Scientists who investigated the scent emitted by the giraffe found 11 separate chemical substances in its fur. The chemicals turned out to have antibiotic properties, having an increased efficiency when combined. Only after a series of experiments can these incredibly complex chemicals be extracted in the laboratory. The giraffe has been using these chemicals to prevent fungi and bacteria, repel ticks, and stop the growth of germs. Where did these tall creatures study chemistry to know how to produce antibiotics such as indole?</p>
<h3><strong>The stubborn doctor</strong></h3>
<p>The bezoar ibex is a type of mountain goat native to Turkey, Iran, Turkmenistan and Pakistan. It has a motley coat of black, brown, grey, reddish-gold, and white. Both the male and female have horns and a goatee. The name means “cure” in Persian, and the locals must have noticed its habit of eating spurge whenever bitten by a snake. Scientists have identified the substance called euphorbone in the spurge plant. Amazingly, an analysis of this substance reveals that certain chemical reactions triggered by euphorbone neutralize the effects of venom. The poisoned creature looks for splurge from among the vegetation, self-medicates, and treats itself free of charge. It sure is no wonder when one realizes that the goat, the snake, and the plant are all created by the same hand.</p>
<h3><strong>The master of diving</strong></h3>
<p>Divers who ascend too quickly to the surface run the high risk of experiencing the bends, an intense pain that is likely to kill because of the gasses coming out of the bloodstream. But how do billions of creatures that lack oxygen tubes lead their entire lives in the sea without experiencing the bends?</p>
<p>Dolphins and whales, for example, descend to depths humans can’t reach on their own and then rise like it is no big deal. Human lungs cannot endure the pressure under such depths, but the bronchi and air sacs in the lungs of dolphins, however, are placed inside a protective cover of special cartilage. To avoid suffering the bends, dolphins release all the air in their lungs before diving deep. But how then do they breathe? The answer is hidden in their muscles, or rather in the myoglobin protein that is available in much higher amounts than in humans. These proteins have the ability to hold in high amounts of oxygen molecules. The much needed oxygen is provided from this source, enabling dolphins and whales to dive as deep as possible.</p>
<h3><strong>Poison for one, food for another</strong></h3>
<p>The macaw is an inhabitant of American tropical regions with an average wing span of 80 cm. It is known to be a tough creature that lives as long as 60 years. The macaw feeds on plants that produce a chemical called strychnine (C<sub>21</sub>H<sub>22</sub>N<sub>2</sub>O<sub>2</sub>), a powerful poison intended to ward off enemies. How can a substance that kills some living things nourish others? Immediately after eating the nutritious but poisonous seeds, the macaw flies to the rocky cliffs in a certain area. When they get there, they gnaw at and swallow some clay-based rock pieces. The fact that the bird ingests clay without any apparent reason is quite an interesting behavior. The reason was revealed only after research into the origins of the behavior. It turns out that the rocks that have clay in them include a substance called kaolinite (Al<sub>2</sub>O<sub>3</sub>.2SiO<sub>2</sub>.2H<sub>2</sub>O) that can absorb the poison in the seeds. The macaw can digest the normally poisonous seeds thanks to this absorption and live on with its life safely. There is no way the macaw can know about the substances present in the clay, so how does it know to eat the clay that can eliminate toxins?</p>
<h3><strong>The antifreeze expert</strong></h3>
<p>The arctic beetle survives against the inhospitable cold of the arctic thanks to a type of alcohol produced in its body that works as antifreeze. The glycerol (C<sub>3</sub>H<sub>8</sub>O<sub>3</sub>), also called glycerin, produced by the insect prevents the blood and other fluid molecules from freezing and thus ice crystals from killing the cells and destroying cellular bonds. Furthermore, the shorter the days and the colder the weather, the more resistant the bodily mechanisms of the arctic beetle become. As the temperature drops, the volume of water in their body is reduced and antifreeze substances such as glycerol and sorbitol are produced in greater amounts. Research on this amazing creature has revealed that it can survive in temperatures as low as -87 degrees Celsius due to glycerol. It is beyond reason to expect an insect to know how to produce an organic compound with the complex formula of C<sub>3</sub>H<sub>8</sub>O<sub>3</sub> and thus protect itself from extreme cold.</p>
<h3><strong>The radiation expert</strong></h3>
<p>Scientists analyzed a surviving scorpion after an atomic bomb test, yet they couldn’t find a satisfying answer to how this animal survived the radiation shower that exterminated all other living organisms. Note that scorpions which came into existence millions of years ago are basically living fossils. Thanks to the protective system they are blessed with, in the past they have survived more powerful solar explosions and harmful radiation from outer space and the sun, and handed down these features to future generations.</p>
<h3><strong>The creature that never feels cold</strong></h3>
<p>The tardigrade, or water bear, is one of the most resistant organisms in nature.</p>
<p>The size of a pinhead, these microorganisms have pin-shaped hoses in their mouth.  These microorganisms have a brain, a pair of eyes, and a digestion system, but they do not have a heart or lungs.  600 different subspecies of the animal have been discovered so far. They feed mostly on moss and lichens and can survive in any environment including space.</p>
<p>They have been observed to survive a temperature of 120 <sup>0</sup>C and a pressure of 1000 atm. In dry environments they contract, causing the water in their tissues to evaporate. During this process, the oxygen consumption of the tardigrade virtually stops. The wind carries the dried tardigrades to other places and when they find a suitable environment (wet moss or humid places) they can come back to life again.</p>
<p>According to Ingemar Jönsson from Kristianstadt University in Sweden who participated in studies on this organism, it is a mystery how these animals survive even when they are subjected to conditions in outer space.</p>
<p>Animals perform amazing tasks with mind-blowing adroitness as if each were an expert chemist. Wondrous mechanisms are activated when a need arises to protect animals from harm. It is wondrous to see how animals can carry out these complex chemical procedures as if they have been instructed at birth.</p>
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		<title>Nuclear Radiation and Misfits of the Standard Model: Neutrinos</title>
		<link>https://fountainmagazine.com/all-issues/2015/issue-103-january-february-2015/nuclear-radiation-january-2015/</link>
		
		<dc:creator><![CDATA[Louima Cunningham]]></dc:creator>
		<pubDate>Thu, 01 Jan 2015 00:00:00 +0000</pubDate>
				<category><![CDATA[Issue 103 (January - February 2015)]]></category>
		<category><![CDATA[antiparticles]]></category>
		<category><![CDATA[cern]]></category>
		<category><![CDATA[chargeless]]></category>
		<category><![CDATA[leptons]]></category>
		<category><![CDATA[light]]></category>
		<category><![CDATA[magazine]]></category>
		<category><![CDATA[mass]]></category>
		<category><![CDATA[model]]></category>
		<category><![CDATA[neutrino]]></category>
		<category><![CDATA[neutrinos]]></category>
		<category><![CDATA[nuclear]]></category>
		<category><![CDATA[Nuclear Radiation]]></category>
		<category><![CDATA[particle]]></category>
		<category><![CDATA[particles]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[Science]]></category>
		<category><![CDATA[sources]]></category>
		<category><![CDATA[standard]]></category>
		<category><![CDATA[universe]]></category>
		<guid isPermaLink="false">http://107.21.79.195/all-issues/2015/issue-103-january-february-2015/nuclear-radiation-january-2015/</guid>

					<description><![CDATA[It would seem nowadays as though the general public&#8217;s knowledge of nuclear radiation is derived less from science and more from science fiction. The beginning of the 20th century brought the atomic age, which in turn brought about considerable anxiety over nuclear radiation. There are a lot of popular sci-fi movies and comic books that [&#8230;]]]></description>
										<content:encoded><![CDATA[<p>It would seem nowadays as though the general public&#8217;s knowledge of nuclear radiation is derived less from science and more from science fiction. The beginning of the 20th century brought the atomic age, which in turn brought about considerable anxiety over nuclear radiation. There are a lot of popular sci-fi movies and comic books that touch upon radiation. As many will remember, when the scientist Dr. Banner triggers a large-scale gamma explosion, he is transformed into a giant green monster in the Hulk. And in the Godzilla franchise, lizards exposed to radiation from a hydrogen bomb turn into giant monsters.</p>
<p><span id="more-1731"></span></p>
<p>However, none of these movies properly &#8211; or accurately &#8211; explains radiation. Regardless of what you do and where you are on a typical day, you are being exposed to millions of particle showers &#8211; another term for radiation &#8211; at all times. Radiation is all around us, but we are not turning into monsters, giants, or any other kind of creature. We do not even sense most of the radiation unless the harmful effects reach the detectable level. In fact, radioactive isotopes (the sources of radiation) found in water, air, soil, and most places in the environment have been emitting radiation since the Big Bang<sup> [1]</sup>, which occurred approximately 14 billion years ago.</p>
<p>Radiation can be emitted by both natural and man-made sources<sup> [2, 3]</sup>. There are generally two main types of natural radiation: radiation from natural sources, such as elements in the ground, is terrestrial, and radiation from outer space, such as charged particles and gamma rays, is cosmic. For example, at this very moment you are being bombarded with cosmic rays every few seconds. On the other hand, the main human-made source of radiation exposure is from medical sources like nuclear medicine, x-rays, computed tomography (CT) scans, etc.</p>
<p>There are various types of radiation emitted by the sun. The most widely recognized forms are visible light, infrared, ultraviolet (UV), x-ray, and gamma radiation. We can only see the visible light, which is defined as having a wavelength on the electromagnetic spectrum between 400-700 nm (a nanometer, or nm, is approximately 10-9 meter). Some of the other kinds of light have greater wavelengths, and some have smaller. In short, visible light&#8217;s region is a very narrow part of the wide EM spectrum.</p>
<p>Why can our eyes see only within this limited range? There are several reasons<sup> [4]</sup>: solar emissions, low absorption in the atmosphere, the energy of chemical bonds, the optical properties of matter, black-body emissions, and so on. Unless all these reasons align into a specific rhythm, we cannot see the kind of light. There are many laws determining light, and the fact that we can see even some light is quite remarkable, and a sign of how perfectly calibrated the universe is.</p>
<h3><b>Misfits of the standard model: Neutrinos</b></h3>
<p>Following our discussion of radiation, I would like to focus on one particular type of radiation: neutrinos. Neutrinos are created in certain types of radioactive decay and nuclear reactions, such as those occurring in the sun. They are one of the most abundant particles in the universe; billions of them pass harmlessly through your body, unnoticed. David Griffiths, a physicist at Reed College, describes neutrinos in his book on particle physics<sup> [5]</sup>:</p>
<p>&#8220;&#8230;neutrinos interact extraordinarily weakly with matter; a neutrino of moderate energy could easily penetrate a thousand light years of lead. That&#8217;s a comforting realization when you learn that hundreds of billions of neutrinos per second pass through every square inch of your body, night and day, coming from the sun.&#8221;</p>
<p>In total, there are three kinds of neutrino flavors, as they are called. These are electron neutrinos, muon neutrinos, and tau neutrinos. Each kind has a tiny mass. According to the Standard Model, there are three kinds of particles in the universe: &#8220;light-weight&#8221; leptons, &#8220;mid-weight&#8221; mesons, and &#8220;heavy-weight&#8221; baryons, such as protons and neutrons. Neutrinos are in the lepton family, which, in total, has only six particles; they have weak interactions within the universe. Neutrinos are neutral leptons since they are chargeless. Other leptons, electron, muon, and tau are called as charged leptons.</p>
<p>The Standard Model is one of the fundamental models in experimental high-energy physics explaining how the universe came into being. Well-known scientists are still improving the model to categorize particles properly in the universe with the aim of finding missing particles. The model explains very well the fundamental forces governing the world: strong nuclear forces, weak nuclear forces, gravitational force, and electroweak force. There were, frankly, two contradictions challenging the Standard Model until today: the Higgs mechanism<sup> [6]</sup> and the mass of neutrinos. The model predicted that Higgs boson<sup> [6]</sup> is the particle responsible for all the mass in the universe. CERN, the biggest particle accelerator<sup>[7]</sup> on earth, announced in July 2012 that they had found a particle that behaves like the Standard Model predicted Higgs boson would. Scientists at CERN are still striving to understand the identity and features of this discovered particle. If they achieve that, they can unravel the mystery and origins of the universe a little bit more. At the end, only the mass of neutrinos will remain a controversial topic within the model.</p>
<p>The Standard Model predicted that neutrinos were chargeless and massless particles. However, cosmic, reactor, and accelerator neutrino experiments, which are the main three experiment types to track neutrinos, confirmed each other on the subject of neutrino oscillation. Neutrino oscillation, in short, means that they can change their flavors. For example, a tau neutrino can convert to an electron neutrino, and vice versa. This discovery shows that these particles can be chargeless but not massless. Each of them has to have small, different masses to be able to perform flavor conversions, according to the laws of physics. That is why these particles are usually called the misfits<sup>[8]</sup> of the Standard Model.</p>
<p>Since each particle was produced with its antiparticle, according to Dirac&#8217;s theory of pairs<sup>[9]</sup>, neutrinos also have their antiparticles, so there are actually six types of neutrinos in the universe. Each antiparticle has exactly the same properties as the original particle, just with the opposite charge. What about the chargeless neutrinos? The difference between neutrinos and antineutrinos is their spin behavior, not their charge. They both have zero charge; however, antineutrinos have a right-handed spin and neutrinos have a left-handed spin.</p>
<p>If each particle has its own antiparticle in theory, there should be the same amount of particles and antiparticles in the universe. However, experimental results show that there are more particles than antiparticles. There are a lot of scientists explaining this dilemma by accepting a parallel universe in which there are more antiparticles than particles, so the total would still be the same. In return, some others are trying to clarify this contradiction by accepting that more particles were created at the beginning of the universe, approximately 14 billion years ago.</p>
<p>Acknowledgment: This article is produced at Mergeous<sup> [10]</sup>, an online article and project development service for authors and publishers dedicated to the advancement of technologies in the merging realms of science and religion.</p>
<h3><b>References</b></h3>
<p>[1] Kaya, A. 2009. &#8220;The Expansion of the Universe and the Big Bang: A Qur&#8217;anic Perspective,&#8221; The Fountain Magazine, Issue 68.<br />[2] <a href="http://en.wikipedia.org/wiki/Radiation">http://en.wikipedia.org/wiki/Radiation<br /></a>[3] <a href="http://www.chem.duke.edu/jds/cruise_chem/nuclear/exposure.html">http://www.chem.duke.edu/jds/cruise_chem/nuclear/exposure.html <br /></a>[4] Why can we see visible light? 2007. Physics Education, 42(1), pp. 37-40.<br />[5] David Griffiths, Introduction to Elementary Particles.<br /> [6] Kara, Cihan. 2013. &#8220;Will CERN Reveal the Origin of the Universe or Cause the End,&#8221; The Fountain Magazine, Issue 92.<br />[7] <a href="http://home.web.cern.ch/">http://home.web.cern.ch/<br /></a>[8] Symmetry Magazine, A Joint Fermilab/SLAC Publication, Spring 2013.<br />[9] Mahmood B. S. 2009. &#8220;The Holy Qur&#8217;an and Dirac&#8217;s Theory of Pairs,&#8221; The Fountain Magazine, Issue 68.<br />[10] Mergeous, Online article and project development platform, <a href="http://www.mergeous.com">http://www.mergeous.com</a></p>
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		<title>What do mosquitoes do when it’s raining?</title>
		<link>https://fountainmagazine.com/all-issues/2012/issue-88-july-august-2012/what-do-mosquitoes-do-when-its-raining-july-augst-2012/</link>
		
		<dc:creator><![CDATA[The Fountain]]></dc:creator>
		<pubDate>Sun, 01 Jul 2012 00:00:00 +0000</pubDate>
				<category><![CDATA[Issue 88 (July - August 2012)]]></category>
		<category><![CDATA[ad 774]]></category>
		<category><![CDATA[c14]]></category>
		<category><![CDATA[cosmic]]></category>
		<category><![CDATA[drop]]></category>
		<category><![CDATA[event]]></category>
		<category><![CDATA[flare]]></category>
		<category><![CDATA[flight]]></category>
		<category><![CDATA[force]]></category>
		<category><![CDATA[high]]></category>
		<category><![CDATA[impact]]></category>
		<category><![CDATA[massive]]></category>
		<category><![CDATA[mosquito]]></category>
		<category><![CDATA[Mosquitoe]]></category>
		<category><![CDATA[mosquitoes]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[raindrops]]></category>
		<category><![CDATA[researchers]]></category>
		<category><![CDATA[Science Square]]></category>
		<category><![CDATA[scientists]]></category>
		<category><![CDATA[small]]></category>
		<category><![CDATA[solar]]></category>
		<category><![CDATA[times]]></category>
		<guid isPermaLink="false">http://107.21.79.195/all-issues/2012/issue-88-july-august-2012/what-do-mosquitoes-do-when-its-raining-july-augst-2012/</guid>

					<description><![CDATA[What do mosquitoes do when it&#8217;s raining? Mosquitoes like climates with high humidity and rainfall. While a single raindrop can weigh 50 times as much as a mosquito, how can mosquitos fly and survive under what seems to be a devastating weather condition for them? Andrew Dickerson and co-workers at Georgia Institute of Technology examined [&#8230;]]]></description>
										<content:encoded><![CDATA[<h3><b>What do mosquitoes do when it&#8217;s raining?</b></h3>
<p>Mosquitoes like climates with high humidity and rainfall. While a single raindrop can weigh 50 times as much as a mosquito, how can mosquitos fly and survive under what seems to be a devastating weather condition for them? Andrew Dickerson and co-workers at Georgia Institute of Technology examined the effects of falling raindrops on the flying mosquitoes using high-speed video capture and found that rain does no damage to flying mosquitoes. Upon impact with mosquitoes, the raindrops do not splash and scatter but they merely deform and hold together. This was calculated to be due to the small diameter and the velocity of the drop. On the other hand, given the relatively small mass of the mosquito, the drop does not significantly alter its speed. A partial hit on the mosquito by the falling drop causes the mosquito to rotate around its flight path. Mosquitoes were found to easily recover and resume their flight immediately after the impact. In the case of a direct hit by a raindrop, the mosquitoes were still able to literally separate themselves from the drop after traveling with the drop for a while without lethal damage and resume flight. The researchers further analyzed the impact force of the raindrops on the mosquitoes and found the direct impact to exert around 80 times the gravitational force. This is an extremely high force for larger organisms however, for mosquitoes with a very strong exoskeleton, this turned out to be a minor fraction of 1500 X g, which the researchers tested the mosquitoes and found them to be still able to fly! The outstanding resilience of such a small organism already inspired scientists to start designing very small robots that may serve as airborne search-and-rescue vehicles. But scientists are still very much limited by the basic factor of how small they can go.</p>
<h3><b>What exactly happened in AD 774?</b></h3>
<p>Researchers in Nagoya University of Japan have recently discovered a cosmic mystery when they were analyzing the growth rings of two cedar trees that are as old as 1200 years. All trees are known to incorporate particles from the atmosphere during photosynthesis. Carbon-14 (C14), one of the exceptional elements in the atmosphere, is generally formed by massive solar flares or by supernovae and it is present in very low percentages. Interestingly, researchers found that the cedar tree ring produced during the growth season of AD 774 had about 1.2% more C14 than in the previous years, that is about 20-times more than the usual range of 0.05%. These results indicate that some cosmic event during AD 774 generated a major influx of radiation leading an excessive amount of C14. Only a massive supernova explosion might have been strong enough to create this much radiation. However, if this was a supernova, we should either be able to catch the traces with modern telescopes, or find historic documents reporting this extraordinary cosmic event. But, we simply have no record of anything unusual happening in our skies in that period. Alternatively, a massive solar flare might have created such a radiation. In fact, 13th-century English chronicler Roger of Wendover mentions a cosmic event that could possibly be a solar flare. However, a flare with that magnitude would have been the biggest solar flare ever recorded by our sun and probably would have destroyed the Earth&#8217;s protective ozone layer leading to disastrous ecological consequences. Thus, the flare hypothesis seems also unlikely. By now, scientists are only positive that some very energetic event occurred in 774. But what exactly was it? Frankly, their guess is as good as ours.</p>
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		<title>Radiotherapy</title>
		<link>https://fountainmagazine.com/all-issues/2009/issue-67-january-february-2009/radiotherapy/</link>
		
		<dc:creator><![CDATA[Louima Cunningham]]></dc:creator>
		<pubDate>Thu, 01 Jan 2009 00:00:00 +0000</pubDate>
				<category><![CDATA[Issue 67 (January - February 2009)]]></category>
		<category><![CDATA[activity]]></category>
		<category><![CDATA[body]]></category>
		<category><![CDATA[cell]]></category>
		<category><![CDATA[disease]]></category>
		<category><![CDATA[diseased]]></category>
		<category><![CDATA[effects]]></category>
		<category><![CDATA[energy]]></category>
		<category><![CDATA[gland]]></category>
		<category><![CDATA[Health & Medicine]]></category>
		<category><![CDATA[iodine]]></category>
		<category><![CDATA[metastases]]></category>
		<category><![CDATA[nuclear]]></category>
		<category><![CDATA[nuclei]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[radioactive]]></category>
		<category><![CDATA[radiopharmaceuticals]]></category>
		<category><![CDATA[radiotherapy]]></category>
		<category><![CDATA[rays]]></category>
		<category><![CDATA[therapy]]></category>
		<category><![CDATA[thyroid]]></category>
		<category><![CDATA[treatment]]></category>
		<guid isPermaLink="false">http://107.21.79.195/all-issues/2009/issue-67-january-february-2009/radiotherapy/</guid>

					<description><![CDATA[As my brother-in-law had some health complaints such as palpitations, insomnia, irritability and excessive sweating, he asked me if I would accompany him to the doctor. As the doctor listened to and examined him, he began to suspect that my brother-in-law might be suffering from hyperthyroidism (excessive activity of the thyroid gland). A test showed [&#8230;]]]></description>
										<content:encoded><![CDATA[<p>As my brother-in-law had some health complaints such as palpitations, insomnia, irritability and excessive sweating, he asked me if I would accompany him to the doctor. As the doctor listened to and examined him, he began to suspect that my brother-in-law might be suffering from hyperthyroidism (excessive activity of the thyroid gland). A test showed that there were excessive thyroid hormones in his blood. The doctor then advised radiotherapy for him instead of removal of his thyroid glands.</p>
<p><span id="more-987"></span></p>
<p>In this treatment, radioactive iodine atoms are administered to the patient. These are absorbed only by cells of the thyroid gland which are then eliminated by the radiation; as a result of this process, the over-activity of the thyroid gland is prevented. By the divine will of God, the All-Healing, the All-Wise, iodine is absorbed only by thyroid cells but not by any other cell-a truly wonderful phenomenon. This treatment is known as the &#8220;bloodless thyroid operation.&#8221;</p>
<p>After he began this treatment, my brother-in-law visited us one day. As soon as she saw him, my small daughter, who loves her uncle very much, ran to him and sat on his lap where she fell asleep after a very short while. But then she woke up within half an hour and suddenly started vomiting. We later understood that the unseen radiation being emitted from the radioactive substance in her uncle’s body first caused my daughter to fall asleep quickly as if she was anesthetized and later had negative effects on her.</p>
<p>Then, an article in a scientific magazine attracted my attention. The concepts of atomic (or nuclear) energy and radiation are usually perceived negatively because of the atomic bombs which were dropped on Nagasaki and Hiroshima or the accident which occurred at the nuclear reactor in Chernobyl. This negative perception has been caused by the sudden deaths of living species, great destruction and the permanent devastating effects observed in the environment after these events. However, the energy within the atomic nucleus also has many potential advantages for humankind. It is just as possible, with this energy, to illuminate houses and work places everywhere as it is to exterminate all the living beings in a city.</p>
<h3><b>Negative effects of radiation</b></h3>
<p>Radiation energy may directly affect molecules within a cell by causing structural disorders especially in its DNA. It also causes ionization of water molecules within a cell and releases free radicals which are harmful to the cell. Damage to molecules and genetic material within a cell may consequently trigger a process that can cause the death of that cell. Thus, it is strongly advised for pregnant women especially to stay away from sources of radiation and also not to expose the body to frequent radiation even for diagnostic purposes, such as X-rays.</p>
<h3><b>Positive effects of radiation</b></h3>
<p>As we consider its beneficial aspects, we realize that nuclear radiation is just one of the innumerable blessings of God. In the field of medicine, for instance, radiation is used to cure diseases like cancer, a disease which, ironically, it sometimes causes. Blood products and medical equipment may be effectively sterilized by the use of radiation. It is also useful in radiological visualization techniques.</p>
<p>Atomic nuclei with unstable composition (radionuclides), which disintegrate without any external interference, display features of radioactivity. The diffusion of energy-bearing rays α, β, γ as a result of this disintegration is called radioactivity and the energy-bearing rays are called radiation. The radioactive substances which are used for the diagnosis and cure of illnesses are known as radioactive medicines or radiopharmaceuticals. This kind of medicine may be composed of pure radioactive nuclei, or they may be compounds which are radioactivated by synthesizing them with radioactive nuclei.</p>
<p>Compared with other radioactive substances, the radiopharmaceuticals used in radiotherapy must have some specific features in terms of radiation type and energy level. Radiopharmaceuticals should be fully absorbed by diseased organ or tissue to be cured and should be applied in such a way that it disseminates the least possible radiation to the rest of the body (so as not to contaminate the body with radiation). That is, the half-life of the radioactive substance should be such that it maintains the correct level of radiation in the tissues to effect the required cure. God has created radioactive substances which emit pure β-rays so that they are ideal for curative purposes.</p>
<h3><b>Radiotherapy</b></h3>
<p>Radioactive nuclear therapy is a treatment for diseased human tissue, usually by the intravenous injection of a suitably formulated radioactive composition. In this treatment, the radioactive composition, when diffused within the body, is held more intensely within the diseased organs, and a kind of radiotherapy at cellular level is thus achieved. The most outstanding example of this kind of therapy is radioactive iodine treatment. This therapy is most frequently applied in cases of excess activity of the thyroid gland in patients with thyroid cancer. As iodine is mostly consumed by the thyroid gland in our body, radioactive iodine (I-131 which is the radioisotope of the element iodine) is particularly suitable for this treatment. The thyroid gland’s feature of absorbing and retaining more iodine than other organs, makes it feasible to treat this organ exclusively by this method when it is diseased. Other peptides marked with particular radioactive nuclei are used in the treatment of other types of cancer and success is observed in some cases. Nuclear therapy is also used in treatment of bone cancers and of pain caused by certain joint diseases.</p>
<h3>Radiopharmaceuticals in palliative treatment of bone pain from metastases</h3>
<p>The spread of cancerous cells from the diseased organ of the body to other organs is called metastasis. Damage and pain originating from osseous (bone) metastases may cause losses in activity and function for the patient. Radiotherapy has long been used particularly in the treatment of limited bone lesions. However, the side effects of radiotherapy are greater since the body areas exposed to X-rays must be increased where there are widespread osseous metastases.</p>
<p>Radiopharmaceutical therapy is useful for patients who have painful metastases throughout multiple osseous zones. In this therapy the patient receives an intravenous injection of suitably formulated radiopharmaceuticals. In this therapy a radioactive substance is used which rapidly leaves the blood circulation system and concentrates within the skeletal system and especially within metastized zones. Radioactive phosphorus has been used for more than thirty years for this purpose.</p>
<h3>Radiopharmaceuticals in therapy for joint disease</h3>
<p>Rheumatoid arthritis, also known as inflammatory joint rheumatism, is one of the most widely seen (approximately 1–2 %) of connective tissue diseases.</p>
<p>In this disease, medication in some cases can become ineffective in the long run and can even be the cause of serious side effects. Radionuclide synovectomy (or radiosynovectomy), which is used in some advanced cases of this disease, yields results close to those obtainable by surgical intervention. It has the additional advantages of being less costly, not necessitating the patient’s hospitalization following the therapy and being repeatable.</p>
<p>It can be seen that the use of this blessing for either favorable (good) or unfavorable (bad) purposes depends on human choice, as is the case for all other divine blessings. Thus, it should be our top priority to use for humanitarian causes the blessing of radiation, which has been bestowed on us for our benefit, but which can seem as if it is harmful at first sight.</p>
<h3><b>Notes</b></h3>
<ol>
<li>Al-Bukhari, &#8220;Tawhid,&#8221; 55; Muslim, &#8220;Tawba,&#8221; 14-16, Ibn Maja, &#8220;Zuhd,&#8221; 35.</li>
<li>Muhammad ibn Ahmad ibn &#8216;Uthman al-Dhahabi, Siyar &#8216;Alam al-Nubala’, 25 vols. (Beirut, 1992), 1:150.</li>
<li>Al-Qushayri, Al-Risala, 133.</li>
<li>In other words, one should regard Him as an All-Merciful and All-Forgiving Lord, rather than as an All-Punishing One.</li>
<li>Al-Bukhari, &#8220;Tawhid&#8221;, 15; Muslim, &#8220;Tawba,&#8221; 1; Al-Tirmidhi, &#8220;Dawa&#8217;at,&#8221; 132.</li>
<li>Al-Qushayri, Al-Risala, 134.</li>
</ol>
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		<title>What Makes the Planets Revolve around the Sun?</title>
		<link>https://fountainmagazine.com/all-issues/2007/issue-60-october-december-2007/what-makes-the-planets-revolve-around-the-sun/</link>
		
		<dc:creator><![CDATA[Louima Cunningham]]></dc:creator>
		<pubDate>Mon, 01 Oct 2007 00:00:00 +0000</pubDate>
				<category><![CDATA[Issue 60 (October - December 2007)]]></category>
		<category><![CDATA[atmosphere]]></category>
		<category><![CDATA[core]]></category>
		<category><![CDATA[corona]]></category>
		<category><![CDATA[earth]]></category>
		<category><![CDATA[energy]]></category>
		<category><![CDATA[field]]></category>
		<category><![CDATA[heat]]></category>
		<category><![CDATA[layer]]></category>
		<category><![CDATA[magnetic]]></category>
		<category><![CDATA[mass]]></category>
		<category><![CDATA[matter]]></category>
		<category><![CDATA[movement]]></category>
		<category><![CDATA[outer]]></category>
		<category><![CDATA[planets]]></category>
		<category><![CDATA[plasma]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[Science]]></category>
		<category><![CDATA[solar]]></category>
		<category><![CDATA[state]]></category>
		<category><![CDATA[sun]]></category>
		<category><![CDATA[zone]]></category>
		<guid isPermaLink="false">http://107.21.79.195/all-issues/2007/issue-60-october-december-2007/what-makes-the-planets-revolve-around-the-sun/</guid>

					<description><![CDATA[The Sun consists of three parts: the interior, the outer layer, and the solar atmosphere. The outer layer of the Sun is similar to the boundary that exists between the Earth and its atmosphere. The core is denser than the outer layer. It is possible to observe the outer layer of the Sun, but it [&#8230;]]]></description>
										<content:encoded><![CDATA[<p>The Sun consists of three parts: the interior, the outer layer, and the solar atmosphere. The outer layer of the Sun is similar to the boundary that exists between the Earth and its atmosphere. The core is denser than the outer layer. It is possible to observe the outer layer of the Sun, but it is not possible to observe the interior. Therefore, any knowledge about the interior of the Sun is dependent on interpretation of data collected about the events that occur on the outer layer. The interior consists of three parts: the core, the radiation zone, and the convection zone. The Sun is made up of matter that is not in a solid, liquid, or gaseous state; rather it is in the plasma state of matter. In the plasma state, due to the very high temperatures, the electrons move away from the nucleus. The elements in this plasma state are charged particles (electrons and protons), which are inclined to react with magnetic and electrical fields. The ionized gas, in the state of plasma, magnetizes the magnetic field of the Sun, increasing its potential by twisting it and forming magnetic field lines. In certain zones in which the magnetic field is strong, the magnetic fields, which are similar in shape to a loop, independently break off and are scattered throughout the solar atmosphere.</p>
<p>More than 99% of the matter in the universe is in a state of plasma. The energy that the Sun distributes comes from the core, which is like a blast furnace; here matter is pure energy or is converted to energy. In the core hydrogen atoms are combined and helium is created through nuclear fusion, which occurs at very high temperatures. During nuclear fusion, enormous amounts of energy are emitted. The total capacity of the Sun’s outer layer that emits energy is around 3.86 x 1,026 watts. However, only 1,368 watt per m<sup>2</sup> comes into the orbit of the Earth. This energy results in the light that we see when we look at the Sun. The core of the Sun is 160 times denser than water on Earth. The temperature in the core is about 15 million °C. If the Sun had not been created at this density and high temperature, such a great amount of energy could not be produced. The energy produced in the core is conveyed to the radiation zone, so called as energy here is conveyed by radiation. The energy produced in the core heats everything while moving to upwards and when it comes close to the outer layer, it loses heat and energy. For instance, there is 1-2 million °C of heat that is dissipated before the end of the radiation zone. At the point where the radiation zone ends, the density of the matter is equal to the density of water on Earth. The energy is conveyed by radiation in the interior part of the Sun, while being conveyed by convection in the outer layer. The source of energy that maintains the light and heat of the Sun is the furnaces at the core. The heat decreases in proportion to the distance from the core. Curiously enough, when moving away from the photosphere (radiation zone) towards the corona, one might think that the temperature in the solar atmosphere should decrease, but in fact it increases. The interior of the corona is almost as hot as the core of the Sun, but the temperature decreases in the outer part of the corona. The cooling process that begins when moving away from the core stops at the corona and the temperature rises from 100,000 °C to 1-5 million °C. Scientists have not yet resolved why the corona has this very high temperature.</p>
<p>The outer layer of the Sun is very stormy. We can compare the events in the outer layer to water boiling in a kettle. This layer is known as the convection zone, which is kept in place by the magnetic field in the corona. The gas pressure in this zone is relatively higher than the magnetic field pressure. Therefore the magnetic field retreats inward and is twisted as a result of the turbulent movements of gas. These movements fulfill the role of enlarging the magnetic field lines of the corona. In the corona, the magnetic field pressure is higher than the gas pressure. It is possible that the extra energy conveyed to the magnetic field is transferred to the plasma in the corona. The energy, in the state of hydromagnetic waves, is squeezed and converted into energy. But we do not know exactly how the energy in the magnetic field is converted to heat in the corona.</p>
<p>The most interesting research topics at the moment are the transfer of energy to the corona and the storage mechanisms for this energy. Matter is heated in the convection zone and expands and rises to the surface. It cools as it rises to the outer layer, becoming denser and then, in a plasma state, sinks down again. This cyclic movement, consisting of a rise and fall, is what is meant by the term “convection.” This movement is conducive to the conveyance of energy from the base of the convection zone to the top. The matter approaching the top cools down and becomes denser here, distributing its energy to the environment. The rising and falling movements of matter in this convection zone are similar to the circular movement observed in water boiling in a kettle. These movements cause the formation of strong magnetic fields in the outer layer of the Sun. <br />The extremely hot gas in the corona moves away from the Sun. When this hot gas mass heads to the planets it is known as “solar wind.” Solar winds are the officers in charge of changes in the climates of planets. This activity in the solar atmosphere causes atmospheric air currents that bring about snow and rain. There are relatively few magnetic fields in the outer layer of the Sun, while there are a number of magnetic fields in the solar atmosphere. The interplanetary magnetic field is formed as a result of the Sun’s magnetic field. Coronal mass ejections expand away from the Sun at speeds that measure as much as 1,250 miles per second. These blasts carry up to ten billion tons of plasma away from the Sun. It may take a few days for the matter, which covers distance at a speed of 60-600 miles per second, to reach the Earth. Solar flares move at the speed of light and can reach the Earth in eight minutes. If coronal mass ejections reach the atmosphere of the Earth, they can create geomagnetic storms. Auroras (radiation that can be observed in Polar zones) are the atmospheric events related to the coronal mass ejections. Large geomagnetic storms can cause electrical power outages and damage communication satellites.</p>
<p>Astronomers record the xrays that emanate from the Sun in the same way that a doctor records the occurrences of pain in patients. It has been discovered that there is a strong correlation between the density of solar flares and the pains of those who suffer migraines. Even if this correlation is statistically meaningful, more controlled research needs to be carried out to understand if there is any biological significance. The storage of magnetic energy in the solar atmosphere and the ejection of the same, like a sudden explosion, cause solar flares. A solar flare occurs when magnetic energy that has built up in the solar atmosphere is suddenly released. During such an explosion, radiation is emitted across virtually the entire electromagnetic spectrum. The amount of energy released is the equivalent of millions of 100-megaton hydrogen bombs exploding at the same time. Considering how just one hydrogen bomb is enough to destroy the entire world, we must thank the All-Powerful God Who placed the Sun at an ideal distance, protecting us both from freezing and burning. The energy released during a flare is typically to the order of 1027 ergs per second. This energy is ten million times greater than the energy released by a volcanic explosion.</p>
<p>The system in which magnetic fields are produced in the Sun can be the cause of some changes on Earth. For example, between the years of 1600 and 1850s solar activities decreased and low temperatures (a minor ice age) were recorded on Earth, especially in much of Europe and North America. Therefore, solar activity carries out its duty on the order of God and works for the adjustment of climates on Earth. It was determined that the temperature differences measured at 6 miles above the North Pole (in the boundary of troposphere/stratosphere) were related to a eleven-year cycle of sunspot explosions. The stratosphere heat over the Polar zones is relatively less cold when the Sun is active, depending on the stratospheric winds. However, the physical mechanisms have not yet been determined.</p>
<h3>How do the planets stay in orbit around the Sun?</h3>
<p>There are two hypotheses on this matter: one of them says that the revolving of the planets around the Sun while they are in their or bit is dependent on the movement around the common mass instead of on the force of gravity. The other theory is that the magnetic field forces, which are created as cycles in the core of the Sun, play an important role in interplanetary gravity. The difference between the hypotheses stems from the structure of the orbits in terms of causes. Circular orbit is formed by the force of gravity, while elliptic orbits are the result of common mass movement. Therefore, it would be more sensible to say that while explaining the phenomenon of planets staying in their orbit around the Sun that a role is played by both common mass movement and matter cycles in the core, reminiscent of the oscillations in the core of the Sun, and the magnetic field that is produced. There are a number of verses in the Qur’an about the Sun and the sky. One of these is: “And the Sun runs the course appointed for it for a term to its resting-place for the stability of it(s system)” (Yasin 36:38). Bediüzzaman Said Nursi says, The Sun is a light-diffusing tree, and the planets are its moving fruits. But unlike trees, the Sun is shaken so that the fruits do not fall. If it were not shaken, they would fall and be scattered.<sup>1</sup></p>
<p>The period of the actual rotation of the Sun is approximately 27 days. The active zones of the sunspots can be observed on the side of the Sun that faces the Earth. The Sun’s movement forms an interesting orbit. Although it is not solid (being in a gas and plasma state), the outer layer of the Sun has different speeds of rotation at different latitudes. Scientists have lately started to use acoustic detectors to receive the signals that emanate from the Sun. The acoustic detectors are used to understand the rising and falling wave movements that this noise causes on the surface of the Sun. Scientists are trying to understand how the sound waves behave in an environment made up of other material, such as oil and vinegar, which form a layer in the water, and they then try to decipher the inner structure of the Sun by making analogies with the events that occur within the Sun. The sound waves that are related to events that occur at the center of the Sun vibrate like a spring. Measurements are made by special acoustic detectors and these reflect the cycles within the Sun. The sound that emanates from the interior parts of the Sun is converted into magnetic waves. These magnetic waves always move, in the form of oscillations that first rise above (to the solar atmosphere) then fall down (to the core of the Sun). The movements within the center of the Sun display rhythmic motions, like water in a pool that has been disturbed. Measuring the smallest sound waves that come from the very core of the Sun, Steven Tomczyk (1994) found that the core of the Sun rotates in a way that is similar to the rotation of the Earth. To put it another way, he found out that the rotation at the core of the Sun occurred independently of latitude and depth, unlike movement in the outer layer of the Sun. While explaining the meaning of the word “li mustaqar” (resting-place) in the Qur’an, Nursi refers to this rotation as follows:</p>
<p>Since the All-Wise Maker operates behind the veil of apparent causality, He has tied the planets to the Sun by His law of gravity and causes them to revolve with distinct but regular motions according to His universal wisdom. To produce gravity, He has made the Sun’s movement on its axis an apparent cause. Thus a resting place means that “the Sun moves in the place determined for it for the order and stability of its own (solar) system.” Like the Divine law, that motion produces heat, heat produces force, and force produces gravity.<sup>2</sup></p>
<p>Some astronomers compare the Sun to a bell that is periodically struck. They also state that the cycles that occur within the Sun and at the outer layer of the Sun play a role in the formation of magnetic fields, gravity forces, and the common mass center of the Sun. As a result of the interconnectivity of all these factors, how the planets revolve around the Sun while staying firmly in their orbits (without being scattered in terms of causes) can be explained. The existence of this huge star and its continuity in a controlled way is a serious matter, which, even though we often take this miracle for granted, must be contemplated. The fact that the Sun is so vital for us, yet that we have no control over it shows us that this fire ball is in the service of humanity thanks to the order of the Divine Will.</p>
<h3>References</h3>
<ul>
<li>http://hesperia.gsfc.nasa.gov/sftheory/cme.htm</li>
<li>http://www.ucar.edu/publications/lasers/sun/what-sun.html</li>
<li>http://athena.wednet.edu/curric/space/sun/sunanat.html</li>
</ul>
<h3>Notes</h3>
<ol>
<li>Nursi, The Words, The Light, Inc., NJ: 2005, p. 413. 2. Ibid.</li>
</ol>
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		<title>God, the Sun, and the Plant</title>
		<link>https://fountainmagazine.com/all-issues/2007/issue-59-july-september-2007/god-the-sun-and-the-plant/</link>
		
		<dc:creator><![CDATA[Louima Cunningham]]></dc:creator>
		<pubDate>Sun, 01 Jul 2007 00:00:00 +0000</pubDate>
				<category><![CDATA[Issue 59 (July - September 2007)]]></category>
		<category><![CDATA[absorption]]></category>
		<category><![CDATA[chlorophyll]]></category>
		<category><![CDATA[color]]></category>
		<category><![CDATA[compound]]></category>
		<category><![CDATA[energy]]></category>
		<category><![CDATA[eye]]></category>
		<category><![CDATA[god]]></category>
		<category><![CDATA[green]]></category>
		<category><![CDATA[human]]></category>
		<category><![CDATA[important]]></category>
		<category><![CDATA[life]]></category>
		<category><![CDATA[Perspectives]]></category>
		<category><![CDATA[photosynthesis]]></category>
		<category><![CDATA[pigment]]></category>
		<category><![CDATA[plant]]></category>
		<category><![CDATA[plants]]></category>
		<category><![CDATA[quanta]]></category>
		<category><![CDATA[quantum]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[ray]]></category>
		<category><![CDATA[solar]]></category>
		<guid isPermaLink="false">http://107.21.79.195/all-issues/2007/issue-59-july-september-2007/god-the-sun-and-the-plant/</guid>

					<description><![CDATA[Have you ever wondered why plants are green? K.A. Timiryazev, a prominent Russian scientist, answered this question first in 1888. In his book, The Sun, Life, and Chlorophyll, Timiryazev argued that green is not the color of plants by coincidence, chlorophyll makes plants green. Moreover, Timiryazev argued, “The green is the key to the cosmic [&#8230;]]]></description>
										<content:encoded><![CDATA[<p>Have you ever wondered why plants are green? K.A. Timiryazev, a prominent Russian scientist, answered this question first in 1888. In his book, The Sun, Life, and Chlorophyll, Timiryazev argued that green is not the color of plants by coincidence, chlorophyll makes plants green. Moreover, Timiryazev argued, “The green is the key to the cosmic role of the plant in nature.” Furthermore, he suggested that plants are programmed not to the visible light, but to energy.</p>
<p>The human eye can identify colors within a 360-760 mm distance. The limits of a curved sight cover the yellow-green field. Every leaf and blade of grass reflects light in this field (540-560 mm), and the human eye can detect thus detect green more clearly than any other color. In other words, God, the All-Knowing, made our eyes see the peaceful and lively color green more easily than other colors, and He granted us the ability to distinct over fifty hues of green – more hues than any other color.</p>
<p>In addition to green, the human eye also perceives the color red, the color of of begonia and barberries, which are colored with antocyan. But there is a chlorophyll layer with its distinctive green under the red layer on top of the leaves. Only a human can see a begonia like this – for example, a bee sees it in black.</p>
<p>Biologists found out that greenblue seaweed, which is really spread all over the world, used to provide our planet with oxygen billions of years ago, contains not only “A”- type chlorophyll, but also other pigments. The human eye, however, is “determined” to see only the green seaweed component created in order to saturate the environment with vital oxygen.</p>
<p>Claiming that “mother nature” has executed such a complicated selection, for the sake of Charles Darwin’s principles, is impossible – it would be more realistic to expect a typewriter to write the encyclopedia Britannica by chance.</p>
<p>We must, however, concede a very important detail. Energy absorption of phototrophic organisms, which is dependant the Sun, is adaptively connected with continuously changing levels of solar radiation. As it is known, the latter comes into soil, which then nourishes plants by facilitating the absorption of energy in a selectively narrow diapason (400-900 to 400- 700 nm). It is impossible to modulate an optimal situation for a plant to be nourished through evolution. A blind evolution would not achieve that in a time span much more time than the multibillion age of our Universe. This leads to the conclusion that the Creator made the specific system of energy absorption in plants via rays projected to the Earth by the Sun.</p>
<p>Aside from the fact that green is created and chosen by God, one more detail deserves listing. Objectively a plant’s leaf and its pigment are connected with selective spectral energy absorption. Emanation with different quanta outside of this precise and narrow “adjustment” could have any influence – negative or positive. Pigment of another kind would not function to fulfill its purpose to be vivifying. Is not turning the ruthless solar radiation into a life-giving flow a manifestation of His wisdom and of the love He has for His creations?</p>
<p>In our everyday life, we engage in amateur garden work or we just admire trees and bushes in bloom. This wonderful event, this miracle, appears to us as something routine. Pigments are highly organized; they are “adjusted” to radiation, which means that their spectrums permit them to absorb radiation in the diapasons at their limit intensity. Moreover, a plant’s organism is always able to increase/decrease this intensity.</p>
<p>For sure, there is one more obvious thing – the issue of the maximum solar radiation is relative. The problem is that according to every scale of wave length, maximum radiation is registered at 578 nm., and at 1015 nm. It would be even more, 1804 nm, if read according to the quantum quantity scale.</p>
<p>From the point of view of basic quantum physics, the most prominent authority on understanding of the role of God in the act of creation, the green color of a leaf is understood to be connected with the features of the pigment itself, the most suitable for the function of absorption and transformation of ray energy.</p>
<p>Another issue is also very important – what determines the diapason of a ray’s energy is its FAR and its photosynthesis diapason accordingly. If we do not accept God as Creator, it is hard to imagine how nature, through all its stages of development led the only source of inner energy, the ATF molecule – through anaerobic, then aerobic breathing and ultimately to all the forms of photosynthesis. This molecule with the energy of its chemical compound in the living system of some 10 Kcal/mole remained in the green plant, but it was not only the breath that was the source of its creation.</p>
<p>I would like to share my observations of over fifty years. As the solar ray energy has become the most important source of energy for plants, simplifying a number of arguments, I can say that the plants are granted a mechanism able to form universal inner quanta divisible to ATF in energy as well as to a photosynthetically important compound named NADP.H (50 kcal/mole each). This is based on the features and spectrum of chlorophyll. The quanta are one of the strongest donors of “his majesty the electron!” Please tell me who will speak of blind evolution after considering these “coincidences”…</p>
<p>I would like to share my observations of over fifty years. As the solar ray energy has become the most important source of energy for plants, simplifying a number of arguments, I can say that the plants are granted a mechanism able to form universal inner quanta divisible to ATF in energy as well as to a photosynthetically important compound named NADP.H (50 kcal/mole each). This is based on the features and spectrum of chlorophyll. The quanta are one of the strongest donors of “his majesty the electron!” Please tell me who will speak of blind evolution after considering these “coincidences”…</p>
<p>“Let all the breathing praise the Lord!”</p>
<p>There is a simple conclusion that could be made from all the above. If such “portions,” or quanta, are formed from solar energy absorbed by plants, then means the primary products of the same type can be also formed. “The quality of light” is of no metabolic importance for the process of synthesis in the limits of ray energy. The Word of God, once spoken out, is realized in a determined way, far distant from Darwinian theory.</p>
<p>Long years of experiments, research, and consultations with colleagues from around the world persuaded this author to change his opinion from vulgar materialism to a deeper understanding. Properties in plants are not the result of “calculabilitive” photosynthesis “touched” by science; like all things, these properties are of a manifestation of His, just as are the lives of humans.</p>
<p>This is the irrational choice of my soul. Nonetheless, as it was admitted in the works on the general problems of science and historic knowledge by the Chief of Department of Civilization Problems at the Russian Academy of Natural Sciences by Prof. V.I. Sheremet -the real breakthrough can be reached with faith in God and exploring the undiscovered. So I offer a second conclusion devoid of materialist explanation. The pigment apparatus of a plant is a complicated chlorophyll-protein complex that functions jointly with its intended object. Who determined this program of compatibility? The plant – the main hero of this article – is given the ability to form a physiological quantum of 50 kcal by itself. Moreover, a high intensity green quantum from outside cannot be used by a separate chlorophyll- protein compound.</p>
<p>The conclusion is obvious and simple: a plant’s life cycle is realized only according to His will and in the regime determined by Him. “Monochromatic” sources of ray energy are not suitable, nor welcomed, by God for the full-fledged artificial raising of plants, but it can be of use for the photosynthesis regulation. So, hotbeds are useful and necessary. The generalized summary is as follows. The green color of leaves and, the blue of the cloudless sky, are not random, they are the work of intelligent design.</p>
<p>So let the green color – the color of plants, of nephrite, malachite, and beryl &#8211; beloved and honored both in the East and in the West. Let the mysterious “green ray” of a seaside sunset, let the green stripe of the rainbow, the bridge to Heaven for the righteous, remain the symbol of His Will, His Life, His Awakening of spring in the peace of the heart.</p>
<p>May peace be with all of you, dear readers! </p>
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		<title>The Search for Gravitational Waves</title>
		<link>https://fountainmagazine.com/all-issues/2003/issue-43-july-september-2003/the-search-for-gravitational-waves/</link>
		
		<dc:creator><![CDATA[Louima Cunningham]]></dc:creator>
		<pubDate>Tue, 01 Jul 2003 00:00:00 +0000</pubDate>
				<category><![CDATA[Issue 43 (July - September 2003)]]></category>
		<category><![CDATA[antenna]]></category>
		<category><![CDATA[antennas]]></category>
		<category><![CDATA[bar]]></category>
		<category><![CDATA[binary]]></category>
		<category><![CDATA[black]]></category>
		<category><![CDATA[detector]]></category>
		<category><![CDATA[detectors]]></category>
		<category><![CDATA[earth]]></category>
		<category><![CDATA[frequency]]></category>
		<category><![CDATA[gravitational]]></category>
		<category><![CDATA[interference]]></category>
		<category><![CDATA[laser]]></category>
		<category><![CDATA[radiation]]></category>
		<category><![CDATA[Science]]></category>
		<category><![CDATA[space]]></category>
		<category><![CDATA[star]]></category>
		<category><![CDATA[stars]]></category>
		<category><![CDATA[time]]></category>
		<category><![CDATA[university]]></category>
		<category><![CDATA[wave]]></category>
		<category><![CDATA[waves]]></category>
		<guid isPermaLink="false">http://107.21.79.195/all-issues/2003/issue-43-july-september-2003/the-search-for-gravitational-waves/</guid>

					<description><![CDATA[Gravitational waves released from cataclysmic events in our galactic neighborhood are 40 orders of magnitude weaker than Coulomb forces and are nearly undetectable on Earth. One order of magnitude is a factor of ten. These waves originate in nature as we speak, having been sent on their way, perhaps thousands or millions of years ago, [&#8230;]]]></description>
										<content:encoded><![CDATA[<p>Gravitational waves released from cataclysmic events in our galactic neighborhood are 40 orders of magnitude weaker than Coulomb forces and are nearly undetectable on Earth. One order of magnitude is a factor of ten. These waves originate in nature as we speak, having been sent on their way, perhaps thousands or millions of years ago, as a result of such distant events as exploding stars (supernovas), coalescing black holes, and less dramatic binary stars in their routine orbiting of each other. Gravitational wave astronomers have developed unique antennas and the associated signal processing hardware to capture these waves, which are described as &#8220;distortions in space-time,&#8221; as opposed to the more customary field terminology of electromagnetics. Unlike radio waves, however, gravitational waves from astronomical sources have not been conclusively detected yet.</p>
<h3><b>Defining the target</b></h3>
<p>Gravitational waves are generated only by the equivalent of a rotating or oscillating system &#8212; that is, two or more masses accelerating toward or away from each other and exhibiting a quadrupole moment of inertia.</p>
<p>Only such quadrupole and higher multipole sources can generate gravitational waves because, whereas there are negative electric charges, there are no negative masses. A negative electric charge oscillating back and forth is the equivalent of a positive charge moving in the opposite direction, and this equivalence enhances the generation of electromagnetic waves. Since there is just one gravitational polarity, however, a mass can oscillate only with respect to a counterweight. This counterweight reacts to the oscillation and generates a gravitational disturbance that almost, but not quite, cancels the disturbance of the body.</p>
<p>As explained by physicist Paul Davies of Australia&#8217;s University of Adelaide, the gravitational disturbances would completely cancel out but for the time required for them to travel between the masses. It is this out-of-phase imbalance in the disturbance&#8217;s cancellation that propagates a gravitational wave. For this reason, such waves are not generated by quiescent stars, those rotating on their axis symmetrically or even exploding symmetrically, because there is no quadrupole moment. However, that situation changes if they explode asymmetrically or change their shape.</p>
<p>On the other hand, a typical binary star system has a quadrupole moment and should produce a slow periodic gravitational wave. A near-enough binary star system would cause a measurable distortion a little in excess of one part in 1021 on Earth.</p>
<p>For the wave to lie in the gravitational-wave detector&#8217;s frequency range (typically 1000 +/-1 Hz.), though, the two stars of the binary must be in the final stage of coalescing, a rare situation. For comparison, a supernova is expected to produce damped exponential impulse waveforms, each of which lasts for 1 millisecond. A collision or collapse of a binary system between two neutron stars, or between a neutron star and a black hole, would produce gravitational waves with a sliding frequency in the 1 to 1000 Hz range, as one star spirals in on its partner.</p>
<h3><b>Why are we searching?</b></h3>
<p>A long time ago, in the Large Magellanic Cloud-one of our Milky Way&#8217;s two companion galaxies, a star exploded. In 1987, 160,000 years later, radiation from that event finally reached Earth. The first to see the brightening star were astronomers in the southern hemisphere.</p>
<p>Scarcely 24 hours earlier, in other parts of the world, other types of detectors had &#8220;seen&#8221; something. At the University of Rome (Italy) and the University of Maryland at College Park (the U.S.), gravitational-wave detectors registered 12 fairly large and about 100 small pulses over a period of 2 hours. Around the same time, the Mont Blanc Neutrino Observatory (France) registered five pulses of neutrinos over a 7-second interval. Similar recordings were made by neutrino detectors in Kamioka, Japan, and Frejus, France.</p>
<p>Astrophysicists are still debating the significance of those observations recorded on Feb. 23 and 24. But others claim the pulses registered in Rome and Maryland may have been due to actual gravitational radiation from an identifiable source &#8212; the supernova of 1987.</p>
<p>Physicists find this ambiguity unsatisfactory. They want to detect the gravitational waves themselves, directly and unequivocally. Indeed, the detection of waves has been called &#8220;the most important of all tests&#8221; of Einstein&#8217;s general theory of relativity by theoretician Kip S. Thorne of the California Institute of Technology (CalTech) in Pasadena. The sensing or reception of gravitational waves also may deepen astronomers&#8217; understanding of the dynamics of such violent events as supernovas, exploding black holes, and the interactions between black holes and neutron stars. As a bonus, whatever is learned about detecting ultra-weak signals might help engineers measuring extraordinarily small displacements or strains.</p>
<p>The understanding, according to Einstein&#8217;s general theory of relativity, is that all objects exist in four-dimensional space-time (that is, in a continuum having three dimensions of space and one of time). The mass of every object curves space-time, a curvature that manifests itself as the gravitational field of the mass. The greater the mass, the greater the curvature of space-time, and the greater the gravitational field.</p>
<p>According to the same theory, massive objects that rotate or explode asymmetrically, or oscillate, give off gravitational waves or ripples that propagate through space-time, like ripples or waves on the surface of the ocean.</p>
<p>Gravitational waves conform to an inverse square law relationship, just like electromagnetic waves. The force of both types of energy declines in proportion to the square of their distance from their source. But gravitational waves are so much weaker than the Coulomb electric force, which renders the detection of such weak waves a monumental challenge to instrumentation.</p>
<p>The evidence that gravitational waves exist is compelling, albeit indirect. The firmest evidence relies on observations made over 7 years by astronomers Joseph Taylor, of Princeton University in New Jersey, and Russell Hulse, then at the University of Massachusetts at Amherst but now also at Princeton. Their measurements of radio waves from a binary pulsar designated PSR1913+16 show that the pulsar&#8217;s 8-hour orbit around the neutron star is gradually contracting; the faster the pulsar revolves around the neutron star, the smaller its orbit gets. As the rate of decrease agrees to within 0.5 percent with predictions derived from the general theory of relativity, the finding is excellent circumstantial evidence for orbital decay being a result of energy lost by gravitational radiation. Even though the gravitational radiation itself was not detected, Taylor and Hulse shared the 1993 Nobel Prize in Physics for this work.</p>
<p>But what would it take to observe the weak gravitational radiation directly? Gravitational waves are generally believed to travel at the speed of light and to deform or distort an object geometrically as they pass through it. For plane-polarized gravitational waves, the two directions are at 45 degrees to each other, not perpendicular as they are for light. In other words, a passing gravitational wave distorts an object first in one direction, then (in the next half-cycle) in another, rotated at a 45-degree angle to the initial direction. It takes another half gravitational wave cycle for the wave to distort at the 90-degree angle characteristic of electro-magnetic waves in the first half-cycle. </p>
<h4><b>Resonant bar detector</b></h4>
<p>In principle, it should be possible to sense this distortion and its after-effects with the aid of strain detectors attached to a suitable &#8220;antenna&#8221; &#8212; a space-time seismometer, if you will. But such an antenna resembles nothing familiar to electrical engineers. In its simplest manifestation, the antenna is a large solid cylindrical bar.</p>
<p>The pioneering resonant-bar detector was designed in the late 1950s and built in the early 1960s by Joseph Weber, professor of physics at the University of Maryland. Weber&#8217;s design called for a mechanically isolated cylinder of solid aluminum weighing several metric tons. Piezoelectric strain transducers attached at intervals around its circumference converted the vibrations induced by any passing gravitational wave into an electric signal. Weber&#8217;s bar resonated mechanically around 1 kHz, so that it would &#8220;ring&#8221; after being distorted by an incoming damped-exponential wave, the shape expected of a gravitational wave from a supernova. Subsequently, other bar detectors were built at many institutions around the world.</p>
<p>The main problem with resonant-bar antennas is their insensitivity. Even the latest of them yield dimensionless strain sensitivities of about one part in 1018 (that is, only 10-18 meter distortion per meter of length), too little to detect gravitational waves from any but the nearest and most violent events. </p>
<h3><b>The laser alternative</b></h3>
<p>The laser interferometer owes its sensitivity in detecting gravitational waves to an arrangement of mirrors suspended on vibration-isolated pendulums. Two pairs of mirrors create two light paths perpendicular to one another. A laser beam is split and the halves sent down each path, rebounding back and forth along the leg between the mirrors hundreds of times before being recombined. The multiple passes create the very long light path required to amplify the gravitational-wave input to detectable amplitude.</p>
<p>In brief, if a gravitational wave passes by, the pendulums holding the mirrors are expected to move a little apart in one leg and a little together in the other leg, in each case by the same tiny fraction of the laser light wavelength. Their movement would shift the relative phase of the two halves of the laser beam, momentarily upsetting the interference patterns that would otherwise be cancelled out. At that instant, the interference pattern would brighten by an amount proportional to the strength of the gravitational wave. The job of monitoring the interference pattern for brightening is handled by electro-optic detectors, which indicate when a passing gravitational wave is detected and which recover its variation over time.</p>
<p>Not only are laser-interferometer detectors potentially more sensitive than resonant-bar antennas, they are also better at detecting a variety of sources because they are inherently broadband. They respond to gravitational waves having a frequency from 10 Hz to 10 kHz, versus the resonant-bar antennas&#8217; 1-Hz bandwidth at 1 kHz. </p>
<h3><b>Input from space</b></h3>
<p>A third and truly exotic method of detecting gravitational waves has been proposed: monitoring the Doppler shift of the carrier frequency (or rather, the retransmission of the tracking station&#8217;s frequency) from two or more interplanetary spacecraft simultaneously. This project is known as LISA (The Laser Interferometry Space Antenna).</p>
<p>The technique is analogous to laser interferometry. The idea is to detect the Doppler shift in a spacecraft&#8217;s microwave frequency as the craft is jostled by a passing gravitational wave &#8212; that is, as space-time is warped in its vicinity.</p>
<p>Inevitably, there are obstacles to overcome. Since the effects of a passing gravitational wave are so small, the reference oscillator must be extremely stable to detect any Doppler shift. Observers must also consider variations in the pressure of the solar wind (which differs from time to time and with the changing distance of the spacecraft from Earth), in forces from the attitude control thrusters (used to occasionally correct the space-craft&#8217;s orientation), and in the refraction of Earth&#8217;s atmosphere (through which the signal must travel). Subtracting all of these variations, the interplanetary detector is expected to have a theoretical sensitivity of about one part in 1016 &#8212; corresponding to a displacement of about 0.065 mm over the shortest distance from Earth to Jupiter, and one-eighth of that over the shortest distance from Earth to Mars. </p>
<h3><b>The noise problem</b></h3>
<p>Noise degrades the sensitivity of any gravitational-wave receiver. The interference is mostly due to seismic activity in the earth, acoustic interference (also known as microphonics) from inhabited surroundings, and heat (thermal noise). Especially troublesome are the non-Gaussian tails of noise distribution, which produce a significant number of false detections.</p>
<p>When a gravitational wave passes through the cylinder and distorts its shape, the moving input coil produces minute changes in the magnetic flux. That magnetic flux change then creates a relatively large variation in the voltage across the SQUID** junctions. In turn, these variations are passed along as voltage signals to succeeding stages of amplification &#8212; generally room-temperature FET amplifiers with optimal filtering for the anticipated signals. If tuned mechanical transformers or resonators are installed between the antenna and the transducer, transfer of the gravitational wave&#8217;s pulse is maximized and amplifier noise coupling is minimized. </p>
<h3><b>Conclusion</b></h3>
<p>Much is being done to achieve a breakthrough in the detection of gravitational waves. A recent High Frequency Gravitational Wave conference held at MITRE Corporation featured proposals and experiment descriptions that could lead to an apparatus that uses gravitational waves for communications. Several large laser interferometer gravitational wave observatories are online and taking data while making sensitivity improvements. The reader is urged to delve further (see references below) to see why there is so much excitement about this new window on the universe. </p>
<h3><b>References</b></h3>
<p>&#8211; Gibbs, W. W. &#8220;Ripples in Spacetime.&#8221; Scientific American, April 2002.</p>
<p>&#8211; Lewis, M. &#8220;Gravitational Waves versus Electromagnetic Wave Antennas.&#8221; IEEE Antennas and Propagation Magazine 37, no. 3, June 1995. Also see http://solo3.abac.com/gwinstitute/.</p>
<p>&#8211; Blair, D. The Detection of Gravitational Waves. Cambridge Univ.: 1991.</p>
<p>&#8211; Boughn, Stephen. &#8220;Detecting Gravitational Waves,&#8221; American Scientist, no. 68. March-April 1980, 174-83. (An overview of the early work in the search for gravitational waves.)</p>
<p>&#8211; Will, Clifford M. Was Einstein Right? New York: Basic Books, 1986. (A readable account of the binary pulsar PSR1913+16 and its role in providing evidence for gravitational waves.)</p>
<p>&#8211; Blair, David G., ed. The Detection of Gravitational Radiation. England and New York: Cambridge Univ. Press, 1991. (Sums up the state of the art in gravitational-wave receivers.)</p>
<p>&#8211; Misner, Charles, Kip S. Thorne, and John Wheeler. Gravitation. W. H. Freeman: 1973. (Still the most used book by students and practitioners in gravitational-wave research.)</p>
<p>&#8211; Thorne, Kip S. Black Holes and Time Warps: Einstein&#8217;s Outrageous Legacy. New York: W. W. Norton, 1994. See chapter 10: &#8220;The Ripples of Curvature,&#8221; which summarizes plans for the Laser Interferometry Gravitational-Wave Observatory (LIGO).</p>
<p>&#8211; E. Amaldi et al. &#8220;Coincidences among the Maryland and Rome Gravitational Wave Detector Data and the Mont Blanc and Kamioka Neutrino Detector in the Period of SN1987A.&#8221; Annals of the New York Academy of Sciences, vol. 571, 1990, 561-76. (Proceedings of the l4th Texas Symposium of Relativistic Astrophysics). (Discusses whether or not gravitational waves were detected along with the first sightings of the 1987 supernova).</p>
<p>&#8211; Grishchuk, Leonid. &#8220;Update on Gravitational Wave Research. Online at Los Alamos&#8217; website on preprints gr-qc/0305051, 13 May 2003. (Provides a more technical treatment.)</p>
<p>** A superconducting quantum interference device (SQUID) is a mechanism used to measure extremely weak signals, such as subtle changes in the human body&#8217;s electromagnetic energy field.</p>
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