{"id":14048,"date":"2023-03-21T02:51:16","date_gmt":"2023-03-21T01:51:16","guid":{"rendered":"https:\/\/www.graviton.at\/letterswaplibrary\/a-note-about-radiation-damage-by-the-red-phoenix-1994\/"},"modified":"2023-03-21T02:51:16","modified_gmt":"2023-03-21T01:51:16","slug":"a-note-about-radiation-damage-by-the-red-phoenix-1994","status":"publish","type":"post","link":"https:\/\/www.graviton.at\/letterswaplibrary\/a-note-about-radiation-damage-by-the-red-phoenix-1994\/","title":{"rendered":"A Note About Radiation Damage By The Red Phoenix (1994)"},"content":{"rendered":"<p>\t\t\tA Note on Radiation Damage<\/p>\n<p>&#8220;There is no safe level of radiation exposure. So the question is not: What<br \/>\n is a safe level? The question is: How great is the risk?&#8221;<\/p>\n<p>\t\t\t\t\t\tKarl Z. Morgan<\/p>\n<p>There have been three major theories as to how radiation damages living<br \/>\ntissue, all set by physicians. All are approximations, and based on broad<br \/>\nassumptions.<\/p>\n<p>(1) The threshold hypothesis: asserts that there exists a safe level of<br \/>\nradiation. The idea behind this thinking is that if the does is low, then<br \/>\nthe cell repair rate is of the order of the damage rate. Hence you get<br \/>\nno resultant damage.<\/p>\n<p>(2) The linear hypothesis: under this theory, you would expect 1 malignant<br \/>\ncancer for 1000 person-rems. For example, you would find one cancerous<br \/>\npatient if you exposed 500 people to 2 rems, or 10000 people to 0.1 rems.<\/p>\n<p>(3) The supralinear hypothesis: the main result here is that for low doses<br \/>\nyou get more cancers\/person-rem than at high doses. Here they not saying you<br \/>\nget more radiation; instead, you get more damaged surviving cells.<\/p>\n<p>\t\t\t\tSome Facts<\/p>\n<p>There are 4 types of ionising radiation. These are alphas<br \/>\n(fast moving helium nuclei),<br \/>\nbetas (electrons), gammas (high energy EM radiation), and neutrons (highly<br \/>\npenetrating).<\/p>\n<p>How does damage occur? In other words, how does radiation cause cancer? <\/p>\n<p>A typical cell is around 0.02mm across, a cell nucleus is about 0.001mm.<\/p>\n<p>When radiation, say a gamma, enters your body, there is a chance it will<br \/>\nintersect with one of your cells. Inside any cell is a nucleus, which<br \/>\ncontains chromosomes. These are essentially DNA helixes. DNA looks like<br \/>\ntwo entwined strings of nucleotides &#8211; the amino acids A, T, C, and G. Across<br \/>\nstrands they are paired A-T and C-G. A portion of DNA (a series of these<br \/>\nacids) is called a gene. Genes exist along chromosomes, and they contain<br \/>\nthe data for proteins.<\/p>\n<p>If the radiation happens to pass into the cell nucleus (which is a relatively<br \/>\nlarge entity compared to the rest of the cell), one of 4 things can happen.<\/p>\n<p>All exposure subjects cells to risk. In order of decreasing probability:<\/p>\n<p>\t\t(1) radiation goes right thru, no interaction.<br \/>\n\t\t(2) radiation does irrepairable destruction, and cell dies.<br \/>\n\t\t(3) radiation does damage to nucleus. Cell survives in<br \/>\n\t\t    this damaged state. After it repetitively divides, it<br \/>\n\t\t    grows into a solid tumour after 30 odd years &#8211; cancer.<br \/>\n\t\t(4) radiation does repairable damage, and cell returns to<br \/>\n\t\t    normal state. (Very low probability).<\/p>\n<p>Possibility (3) is the one to watch out for. During division, the DNA<br \/>\nstrands stretch out, and it is during this time which your cells are most<br \/>\nsusceptible to damage.<\/p>\n<p>It is also possible for the radiation to ionise the water in the cell<br \/>\ncytoplasm, leading to the formation of free radicals, which can travel<br \/>\nsome distance. They can react chemically with the DNA in the nucleus,<br \/>\ninterfering with the chemical bonding along the helix. <\/p>\n<p>Two types of damaging interaction can occur with the amino acids.<\/p>\n<p>\t\t(a) point mutations<br \/>\n\t\t\t&#8211; deletion<br \/>\n\t\t\t&#8211; substitution<br \/>\n\t\t\t&#8211; inversion<br \/>\n\t\t\t&#8211; addition<\/p>\n<p>\t\t(b) large scale mutations (chromosome aberrations)<br \/>\n\t\t\t&#8211; deletion e.g. retinoblastoma<br \/>\n\t\t\t&#8211; amplification<br \/>\n\t\t\t&#8211; translocation<\/p>\n<p>It is also possible to have compound breaks along the DNA, which is not<br \/>\neasy for the cell to repair, unlike single strand or double strand breaks.<\/p>\n<p>The cell and nuclear membranes are also susceptible to damage. This could<br \/>\nbe due to alterations in permeability\/osmosis in the membrane due to the<br \/>\nradiation-induced imbalance of ionised particles.<\/p>\n<p>Once a certain threshold is exceeded, you will start saturating the cells.<br \/>\nThis lethal threshold serves to define two categories of radiation.<\/p>\n<p>\t\t\t\tEffects<\/p>\n<p>EFFECT\t\tNATURE\t\t\tTHRESHOLD?\tDOSE DEPENDENCE<\/p>\n<p>Stochastic\tNon-lethal mutations\tNo\t\tProbability of<br \/>\n(somatic or\taffecting single cells \t\t\teffect increases<br \/>\ngenetic)\t\t\t\t\t\twith dose<\/p>\n<p>Deterministic\tLethal mutations\tYes\t\tSeverity of<br \/>\n\t\taffecting large number\t\t\teffect increases<br \/>\n\t\tof cells\t\t\t\twith dose<\/p>\n<p>\t\t\t\tCancer<\/p>\n<p>Stem cells are ones which are able to undergo mitosis when the human body<br \/>\nhas reached full maturity. Examples are blood cells, and the cells lining<br \/>\nyour intestines. During normal functioning of your body, cell replacement<br \/>\nbalances cell loss.<\/p>\n<p>In cancer, a stem fails to stop its mitosis. It and its descendants divide<br \/>\nuncontrolled, forming a tumour. A bit like a binary tree in cell<br \/>\nmultiplicity.<\/p>\n<p>Oncogenes are genes which interfere with the cell division process. They<br \/>\nare mutations of proto-oncogenes, whose role are to control cell growth<br \/>\nand mitosis. It is thought radiation promotes creation of oncogenes.<\/p>\n<p>There are also cancer-suppressing genes, which inhibit oncogene formation.<br \/>\nThe best known example is the Rb gene, which inhibits retinoblastoma.<\/p>\n<p>After all of this, let me add a fourth idea on radiation damage:<\/p>\n<p>(4) probability of hereditary genetic damage or cancer is a function of:<\/p>\n<p>type of radiation (a,b,g,n) x energy of radiation x dose rate<\/p>\n<p>Here you have 4 discrete degrees of freedom, and 2 continuous degrees: rate &amp;<br \/>\nenergy. Assume that there is a cut-off energy for a unit of a particular type<br \/>\nof radiation, E_max, such that if E &gt; E_max a cell will die, and E &lt; E_max<br \/>\nthe cell will survive (either in damaged or undamaged state). We are worried<br \/>\nabout the E  E_max then you get radiation poisoning and<br \/>\nyou will definitely die if you get a large enough dose.<\/p>\n<p>The probability of nucleus intersection is a function of radiation type. (The<br \/>\nsize of radiation varies considerably.)<\/p>\n<p>The probability of a nucleus being hit twice or more is very low, unless<br \/>\nthe number of incident radiation approaches the sample size. In which case<br \/>\nyou get radiation poisoning and die anyway.<\/p>\n<p>You get a 6D phase space of statistical mechanics. Supplement this with an<br \/>\naction in path integral form. Plotted, you&#8217;d have a 6D graph, unlike your<br \/>\nnormal 3D graphs. It&#8217;s worse than the 4D spacetime of general relativity.<br \/>\nNo wonder the physicicans only plot projections! You can trace out a person&#8217;s<br \/>\nhistory in this phase space, and then give them a final probability of<br \/>\ncancer\/hereditary damage.<\/p>\n<p>============================================================================<\/p>\n<p>Plutonium&#8217;s Risk to Human Health Depend On Its Form<\/p>\n<p>In a nuclear explosium, plutonium-239 fissions and releases a huge amount of<br \/>\nenergy and radiation. But plutonium itself is a highly toxic element that requires<br \/>\na great deal of care in handling.<\/p>\n<p>Experts agree that the silvery, unstable metal plutonium-239, with a half-life of<br \/>\n24,000 years, is hazardous and sould be isolated from the biosphere. However, the<br \/>\nrisks posed to workers and communities by stored plutonium depend on the route of<br \/>\nexposure as well as the particle size, isotope, and chemical form.<\/p>\n<p>Weapons-grade plutonium outside the body presents little risk unless exposures are<br \/>\nfrequent and extensive. It emits primarily alpha particles, which cannot penetrate<br \/>\nskin, clothing, or even paper. Nearly all the energy from plutonium is deposited<br \/>\non the outer, nonliving layer of the skin, where it causes no damage. The neutrons<br \/>\nand the relatively weak gamma photons it emits can penetrate the body, but large<br \/>\namounts of weapons-grade plutonium would be needed to yield substantial doses.<\/p>\n<p>Workers wearing only lead aprons can handle steel drums containing solid plutonium<br \/>\nmetal with no immediate untoward effects. However, as weapons-grade plutonium<br \/>\nages, it becomes more dangerous because some of the contaminating plutonium-241 is<br \/>\nconverted via beta decay to americium-241, which emits far stronger gamma<br \/>\nradiation.<\/p>\n<p>On the other hand, plutonium inside the body is highly toxi. Solid plutonium metal<br \/>\nis neither easily dispersed nor easily inhaled or absorbed into the body. But if<br \/>\nplutonium metal is exposed to air to any degree, it slowly oxidizes to plutonium<br \/>\noxide (PuO2), which is a powdery, much more dispersable substance. Depending on<br \/>\nthe particle size, plutonium-239 oxide may lodge deep in the alveoli of the lung<br \/>\nwhere it has a biological half-life of 500 days, and alpha particles from the<br \/>\nopxide can cause cancer. Also, fractions of the inhaled plutonium oxide can slowly<br \/>\ndissolve, enter the bloodstream, and end up primarily in bone or liver.<\/p>\n<p>Plutonium oxide is weakly soluble in water. If it is ingested in food or water,<br \/>\nonly a small fraction (4 parts per 10,000) is absorbed into the gastrointestinal<br \/>\ntract. However, it may take just a few millionths of a gram to cause cancer over<br \/>\ntime. In animals, small doses induce cancer, especially in lung and bone.<\/p>\n<p>In published studies of plutonium&#8217;s effects on humans, most subjects were exposed<br \/>\nto multiple sources of radiation. Some researchers say the available health data<br \/>\non plutonium workers have not yet been used to do careful epidemiological studies,<br \/>\nbecause researchers have been denied access to much of the data on workers and<br \/>\nmilitary personnel exposed to plutonium. In the studies done so far, plutonium<br \/>\nworkers do not show major excesses of any type of cancer.<\/p>\n<p>Becuase of the relative lack of human data, the risks of chronic exposure to<br \/>\nplutonium are uncertain. Exposure standards in the U.S. are based partly on<br \/>\nstudies of survivors of Hiroshima and Nagasaki and partly on animal experiments. A<br \/>\n1991 White House Office of Science &amp; Technology Policy studye says that<br \/>\n&#8220;sufficient human data are not available to provide accurate risk assessment of<br \/>\nexposure.&#8221;<\/p>\n<p>============================================================================<\/p>\n<p>\t\t\tNuclear Blast Effects<\/p>\n<p>The first thing bomb victims experience is the intense flux of photons from<br \/>\nthe blast, which releases 70-80% of the bomb&#8217;s energy. See the Hiroshima-<br \/>\nNagasaki file for first hand accounts. The effects go up to third degree<br \/>\nthermal burns, and are not a pretty sight. Initial deaths are due to this<br \/>\neffect.<\/p>\n<p>Then next phenomenon is the supersonic blast front. You see it before you<br \/>\nhear it. The pressure front has the effect of blowing away anything in its<br \/>\npath. Heavy steel girders were found bent at 90 degree angles after the<br \/>\nJapanese bombings. <\/p>\n<p>After the front comes the overpressure phase. It would feel like being under<br \/>\nwater a few hundred metres. At a few thousand metres under the sea, pressurised<br \/>\nhulls implode. The pressure gradually dies off, and there is a negative<br \/>\noverpressure phase, with a reversed blast wind. This reversal is due to<br \/>\nair rushing back to fill the void left by the explosion.<\/p>\n<p>The air gradually returns to room pressure. At this stage, fires caused by<br \/>\nelectrical destruction and ignited debris, turn the place into a firestorm.<br \/>\nJust like Dresden in WWII. It is estimated over fifty thousand died in the<br \/>\nfirst few days of the Hiroshima bombing.<\/p>\n<p>Then come the middle term effects such as keloid formation and retinal<br \/>\nblastoma.<\/p>\n<p>Genetic or hereditary damage can show up up to forty years after initial<br \/>\nirradiation.<\/p>\n<p>The following diagram is of blast zone radii, courtesy of Outlaw Labs.<br \/>\nNote that damage from blast pressure falls off as a function of 1\/r^3.<\/p>\n<p>============================================================================<\/p>\n<p>                &#8211; Breakdown of the Atomic Bomb&#8217;s Blast Zones &#8211;<br \/>\n                &#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-<\/p>\n<p>                                       .<br \/>\n                         .                           .<\/p>\n<p>              .                        .                        .<br \/>\n                             .                   .<br \/>\n               [5]                    [4]                    [5]<br \/>\n                                       .<br \/>\n                      .        .               .        .<\/p>\n<p>       .                  .                         .                  .<\/p>\n<p>                 .          [3]        _        [3]          .<br \/>\n                      .           .   [2]   .           .<br \/>\n                                .     _._     .<br \/>\n                               .    .~   ~.    .<br \/>\n    .          . [4] .         .[2].  [1]  .[2].         . [4] .          .<br \/>\n                               .    .     .    .<br \/>\n                                .    ~-.-~    .<br \/>\n                      .           .   [2]   .           .<br \/>\n                 .          [3]        &#8211;        [3]          .<\/p>\n<p>       .                  .                         .                  .<\/p>\n<p>                      .        ~               ~        .<br \/>\n                                       ~<br \/>\n               [5]           .        [4]        .           [5]<br \/>\n                                       .<br \/>\n              .                                                 .<\/p>\n<p>                         .                           .<br \/>\n                                       .<\/p>\n<p> ============================================================================<\/p>\n<p>                              &#8211; Diagram Outline &#8211;<br \/>\n                             &#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;<\/p>\n<p>     [1]  Vaporization Point<br \/>\n          &#8212;&#8212;&#8212;&#8212;&#8212;&#8212;<br \/>\n          Everything is vaporized by the atomic blast.  98% fatalities.<br \/>\n          Overpress=25 psi.  Wind velocity=320 mph.<\/p>\n<p>     [2]  Total Destruction<br \/>\n          &#8212;&#8212;&#8212;&#8212;&#8212;&#8211;<br \/>\n          All structures above ground are destroyed.  90% fatalities.<br \/>\n          Overpress=17 psi.  Wind velocity=290 mph.<\/p>\n<p>     [3]  Severe Blast Damage<br \/>\n          &#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-<br \/>\n          Factories and other large-scale building collapse.  Severe damage<br \/>\n          to highway bridges.  Rivers sometimes flow countercurrent.<br \/>\n          65% fatalities, 30% injured.<br \/>\n          Overpress=9 psi.  Wind velocity=260 mph.<\/p>\n<p>     [4]  Severe Heat Damage<br \/>\n          &#8212;&#8212;&#8212;&#8212;&#8212;&#8212;<br \/>\n          Everything flammable burns.  People in the area suffocate due to<br \/>\n          the fact that most available oxygen is consumed by the fires.<br \/>\n          50% fatalities, 45% injured.<br \/>\n          Overpress=6 psi.  Wind velocity=140 mph.<\/p>\n<p>     [5]  Severe Fire &amp; Wind Damage<br \/>\n          &#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-<br \/>\n          Residency structures are severely damaged.  People are blown<br \/>\n          around.  2nd and 3rd-degree burns suffered by most survivors.<br \/>\n          15% dead.  50% injured.<br \/>\n          Overpress=3 psi.  Wind velocity=98 mph.<\/p>\n<p>&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-<\/p>\n<p>                            &#8211; Blast Zone Radii &#8211;<br \/>\n                           &#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-<br \/>\n                          [3 different bomb types]<br \/>\n____________________________________________________________________________<br \/>\n  ______________________   ______________________   ______________________<br \/>\n |                      | |                      | |                      |<br \/>\n |    -[10 KILOTONS]-   | |     -[1 MEGATON]-    | |    -[20 MEGATONS]-   |<br \/>\n |&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-| |&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-| |&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;-|<br \/>\n | Airburst &#8211; 1,980 ft  | | Airburst &#8211; 8,000 ft  | | Airburst &#8211; 17,500 ft |<br \/>\n |______________________| |______________________| |______________________|<br \/>\n |                      | |                      | |                      |<br \/>\n |  [1]  0.5 miles      | |  [1]  2.5 miles      | |  [1]  8.75 miles     |<br \/>\n |  [2]  1 mile         | |  [2]  3.75 miles     | |  [2]  14 miles       |<br \/>\n |  [3]  1.75 miles     | |  [3]  6.5 miles      | |  [3]  27 miles       |<br \/>\n |  [4]  2.5 miles      | |  [4]  7.75 miles     | |  [4]  31 miles       |<br \/>\n |  [5]  3 miles        | |  [5]  10 miles       | |  [5]  35 miles       |<br \/>\n |                      | |                      | |                      |<br \/>\n |______________________| |______________________| |______________________|<br \/>\n____________________________________________________________________________<\/p>\n<p>============================================================================<\/p>\n<p>\t\t\tAtmospheric Effects of Blasts<\/p>\n<p>The Mushroom Cloud<\/p>\n<p>The heat from fusion and fission instantaneously raises the surrounding air<br \/>\nto 10 million degrees C. This superheated air plasma gives off so much light<br \/>\nthat it looks brighter than the sun, and is visible hundreds of kms away.<br \/>\nThe resultant fireball quickly expands. It is made up of hot air, and hence<br \/>\nrises, at a rate of a few hundred metres per second. After a minute or so,<br \/>\nthe fireball has risen to a few kilometres, and has cooled off to the extent<br \/>\nthat it no longer radiates.<\/p>\n<p>The surrounding cooler air exerts some drag on this rising air, which slows<br \/>\ndown the outer edges of the cloud. The unimpeded inner portion rises a bit<br \/>\nmore quicker than the outer edges. A vacuum effect occurs when the outer<br \/>\nportion occupies the vacuum left by the higher inner portion. The result is<br \/>\na smoke ring. <\/p>\n<p>The inner material gradually expands out into a mushroom cloud, due to<br \/>\nconvection. If the explosion is on the ground, dirt and radioactive debris<br \/>\nget sucked up the stem, which sits below the fireball.  <\/p>\n<p>Collisions and ionisation of the cloud particles result in lightning bolts<br \/>\nflickering to the ground. <\/p>\n<p>Initially, the cloud is orange-red due to nitrous oxide formation (cf car<br \/>\nsmog). This reaction happens whenever air is heated.<\/p>\n<p>When the cloud cools to air temperature, the water vapour starts to<br \/>\ncondense. The cloud turns from red to white.<\/p>\n<p>In the final stages, the cloud can get about 100km across and 40km high,<br \/>\nfor a megaton class explosion.<\/p>\n<p>============================================================================<\/p>\n<p>\t\t\tElectromagnetic Pulse (EMP)<\/p>\n<p>A nuclear explosion gives off radiation at all wavelengths of light. Some<br \/>\nis in the radio\/radar portion of the spectrum &#8211; the EMP effect. The EMP<br \/>\neffect increases the higher you go into the atmosphere. High altitude<br \/>\nexplosions can knock out electronics by inducing a current surge in<br \/>\nclosed circuit metallic objects &#8211; computers, power lines, phone lines,<br \/>\nTVs, radios, etc. The damage range can be over 1000km.<\/p>\n<p>============================================================================<\/p>\n<p>Here are some good references on radiation damage. See also the main<br \/>\nReferences file.<\/p>\n<p>AUTHOR:     Sumner, David, D. Phil<br \/>\nTITLE:      Radiation risks : an evaluation \/ David Sumner, Tom Wheldon, Walter<br \/>\n            Watson. &#8212; 3rd ed.<br \/>\nISBN\/ISSN:  187078104X<br \/>\nIMPRINT:    Glasgow [Scotland], Tarragon Press, 1991<br \/>\nPHYS DESC:  236 p., ill., map, 21 cm.<br \/>\nADD AUTH1:  Wheldon, Tom<br \/>\nADD AUTH2:  Watson, Walter<br \/>\nNOTE 1:     Includes index Bibliography: p. 227-229<br \/>\nSUBJECT 1:  Radiation&#8211;Physiological effect<br \/>\nSUBJECT 2:  Cells&#8211;Effect of radiation on<br \/>\n[Good introductory work.]<\/p>\n<p>CALL NO:    Me f 616.989707 LOW<br \/>\nTITLE:      Low-level radiation effects: a fact book: prepared by Subcommittee<br \/>\n            on Risks of Low-Level Ionizing Radiation: A. Bertrand Brill &#8230; [et<br \/>\n            al.]<br \/>\nISBN\/ISSN:  0932004148<br \/>\nIMPRINT:    New York, NY: Society of Nuclear Medicine: c1982-<br \/>\nPHYS DESC:  1 v. (loose-leaf): ill: 30 cm.<br \/>\nADD AUTH1:  Brill, A. Bertrand<br \/>\nADD AUTH2:  Society of Nuclear Medicine. Subcommittee on Risks of Low-Level<br \/>\n            Ionizing Radiation<br \/>\nNOTE 1:     To be kept up to date by inserts<br \/>\nSUBJECT 1:  Ionizing radiation&#8211;Physiological effect<br \/>\nSUBJECT 2:  Ionizing radiation&#8211;Toxicology<br \/>\nSUBJECT 3:  Radiation injuries<br \/>\nSUBJECT 4:  Low-level radiation&#8211;Physiological effect<\/p>\n<p>CALL NO:    Me 574.1915 BIOL<br \/>\nTITLE:      Biological effects of low-level radiation : proceedings of an<br \/>\n            international symposium on the effects of low-level radiation with<br \/>\n            special regard to stochastic and non-stochastic effects \/ jointly<br \/>\n            organized by the International Atomic Energy Agency and the World<br \/>\n            Health Organisation, and held in Venice, Italy, 11-15 April 1983<br \/>\nISBN\/ISSN:  9200101836<br \/>\nIMPRINT:    Vienna, International Atomic Energy Agency, 1983<br \/>\nPHYS DESC:  682 p., ill, 24 cm.  (Proceedings series)<br \/>\nADD AUTH1:  International Atomic Energy Agency<br \/>\nADD AUTH2:  World Health Organization<br \/>\nSERIES 1:   Proceedings series (International Atomic Energy Agency)<br \/>\nNOTE 1:     English and French<br \/>\nSUBJECT 1:  Radiation&#8211;Toxicology&#8211;Congresses<br \/>\nSUBJECT 2:  Radiation&#8211;Physiological effect&#8211;Congresses<\/p>\n<p>CALL NO:    DS 574.1915 KIEF<br \/>\nAUTHOR:     Kiefer, J (Jurgen) , 1936-  [Biologische Strahlenwirkung. English]<br \/>\nTITLE:      Biological radiation effects \/ Jurgen Kiefer<br \/>\nISBN\/ISSN:  3540510893<br \/>\nIMPRINT:    Berlin, New York, Springer-Verlag, c1990<br \/>\nPHYS DESC:  xvii, 444 p., ill, 24 cm.<br \/>\nNOTE 1:     Rev. translation of: Biologishce Strahlenwirkung Includes<br \/>\n            bibliographical references (p. [415]-435) and indexes<br \/>\nSUBJECT 1:  Radiobiology<br \/>\nSUBJECT 2:  Radiation&#8211;Physiological effect<br \/>\nSUBJECT 4:  Radiation protection<\/p>\n<p>To learn more about air explosions, see the Reference by Kinney and Graham,<br \/>\n&#8220;Explosive Shocks in Air&#8221;.<\/p>\n<p>The Red Phoenix, 1994.<\/p>\n<div class='watch-action'><div class='watch-position align-right'><div class='action-like'><a class='lbg-style1 like-14048 jlk' href='javascript:void(0)' data-task='like' data-post_id='14048' data-nonce='41b6e01389' rel='nofollow'><img class='wti-pixel' src='https:\/\/www.graviton.at\/letterswaplibrary\/wp-content\/plugins\/wti-like-post\/images\/pixel.gif' title='Like' \/><span class='lc-14048 lc'>0<\/span><\/a><\/div><\/div> <div class='status-14048 status align-right'><\/div><\/div><div class='wti-clear'><\/div>","protected":false},"excerpt":{"rendered":"<p>A Note on Radiation Damage &#8220;There is no safe level of radiation exposure. So the question is&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7],"tags":[27],"class_list":["post-14048","post","type-post","status-publish","format-standard","hentry","category-othernonsense","tag-english","wpcat-7-id"],"_links":{"self":[{"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/posts\/14048","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/comments?post=14048"}],"version-history":[{"count":1,"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/posts\/14048\/revisions"}],"predecessor-version":[{"id":14049,"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/posts\/14048\/revisions\/14049"}],"wp:attachment":[{"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/media?parent=14048"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/categories?post=14048"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.graviton.at\/letterswaplibrary\/wp-json\/wp\/v2\/tags?post=14048"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}