| Home Page | Overview | Site Map | Index | Appendix | Illustration | About | Contact | Update | FAQ |
![]() |
Nuclear weapons are similar to those of more conventional types in so far as their destructive action is due mainly to blast or shock. On the other hand, there are several basic differences between nuclear and high-explosive weapons. In the first place, nuclear explosions can be many thousands (or millions) of times more powerful than the largest conventional detonations. Second, a fairly large proportion of the energy in a nuclear explosion is emitted in the form of light and heat, generally referred to as "thermal radiation". It is capable of causing skin burns and of starting fires at considerable distances. Third, the nuclear explosion is accompanied by highly penetrating and harmful invisible rays, called the "initial nuclear radiation". Finally, the substances remaining after a nuclear explosion are radioactive, emitting similar radiations over an extended period of time. This is know as the "residual nuclear radiation" or "residual radioactivity". Figure 14-15a shows the distribution of energy in a typical nuclear explosion. The detonation of nuclear weapon leads to the liberation |
Figure 14-15a Distribution of Energy [view large image] |
of a large amount of energy in a very small period of time within the casing. Tre-mendous pressures (over million times the ambient pressure) is produced in the form of shock wave. Damage is done at the shock front by the huge difference in air pressure as well as by the drag force (strong winds) trailing behind. The radiation energy are absorbed within a few feet |
![]() |
![]() |
4.5 miles. As the shock wave travels in the air away from its source, the overpressure at the front steadily decreases, and the pressure behind the front falls off until it develops a "negative pressure", in which a partial vacuum is produced and the air is sucked in reversing the wind direction. Figure 14-15c illustrates the variation of overpressure with distance at successive times. Its effects on a light structure, a tree, and a small animal are indicated with a series of pictures corresponding to the various |
Figure 14-15b Mushroom Cloud [view large image] |
Figure 14-15c Shock Wave [view large image] |
times. Speed of the shock front varies from about 1600 ft/sec initially to 1150 ft/sce (slightly faster than the sound speed of 1115 ft/sec) at later time. |
![]() |
the behavior of DNA and RNA is modified. There are consequently changes in the cells which may have significant detectable effects on the body as a whole. All radiations apparently induce the same general biological consequences, but neutrons are unusual in the respect that they can convert a N-14 atom in an amino acid into one of C-14. Such a change might inactivate an enzyme or affect a nucleic acid. Certain macroscopic phenomena are soon apparent in the living cell. Among these are breaking of the chromosomes. Figure 14-15d shows the normal plant cell, |
Figure 14-15d Biological Effects [view large image] |
with two groups of chromosomes (left), and changes (right) produced by X-rays. Frequently, the cells are unable to undergo mitosis, so that normal replacement occurring in the living organism is inhibited. |
![]() |
![]() |
debris of buildings collapsed by the shock wave, and acute exposure to the high radiation. Beyond the immediate blast area, casualties are caused from the heat, radiation, and fires spawned from the heat wave. Figure 14-15f presents two views of Hiroshima before and after an atomic-bomb attack. It occurred in the morning (8:16 a.m.) of August 6, 1945. The bomb detonated at an altitude of 580 meters killing or wounding about half of its 350,000 inhabitants with long-term effects on |
Figure 14-15e Effects of A-Bomb |
Figure 14-15f Hiroshima |
incalculable numbers among the survivors. |
![]() |
![]() |
Figure 14-16a shows the symptoms of radiation sickness according to the dose received. The radiation unit in Roentgen was originally defined in 1928. It is the energy to produce 2.1 x 109 ion pairs in a volume of 1 cubic centimetre of air, which is |
Figure 14-16a Radiation Sickness [view large image] |
Figure 14-16b Sick Survivor |
equivalent to about 100 ergs per gram of water or tissue irradiated. Although it seems to be a minute amount of energy |
![]() |
radiation exposure at the median level of 500 rad and the lower level of 100 rad, which is variably expressed as rem or r and is equal to 0.0838 Roentgen. In the U.S., the National Institute of Standard and Technology (NIST) strongly discourages the use of Roentgen as it is not really a SI unit. Another SI unit called Sievert (Sv = 1 J/kg) is also widely used in medical circle to measure the biological effects (1 rad = 0.01 Sv = 10 mSv). Figure 14-16c lists the adverse symptoms related to the levels of radiation (in mSv). Table 14-07 is a short list of the radioactive isotopes and uptakes by various organs. The gamma rays emitters can be expelled out of the body and is super-scripted by the symbol "*". For example, Cs-137 has a half life of 30 years, but half of the substance would be removed from the body in 70 days. |
Figure 14-16c Effects of Radiation [view large image] |
| Radioactive Isotope | Half Life | Targeted Organ |
|---|---|---|
| I-131 (Iodine)* | 8.3 days | Thyroid | Rn-222 (Radon) Pu-239 (Plutonium) Kr-85 (Krypton)* |
3.8 days 24,000 years 10 years |
Lung, (Rn-222 tends to spread over the whole body) |
Co-60 (Cobalt) Pu-239 (Plutonium) |
5.3 years 24,000 years |
Liver | U-235 (Uranium) U-238 (Uranium) Pb-210 (Lead) Ru-106 (Ruthenium)* |
700,000,000 years 4,500,000,000 years 22.3 years 1 year |
Kidney | Cs-137 (Cesium)* K-42 (Potassium)* C-14 (carbon) T-3 (Tritium) S-35 (Sulfur) |
30 years 12 hours 5730 years 12.2 years 87 days |
Skin, muscle | Pu-239 (Plutonium) Sr-90 (Strontium) Ra-226 (Radium) |
24,000 years 28.8 years 1620 years |
Bone | Po-210 | 138 days | Spleen (high toxicity) | Pu-239 (Plutonium) | 24,000 years | Gonads | K-42*, Co-60*, Kr-85*, I-131*, Cs-137*, Pu-239 |
12 hours - 24,000 years |
Ovaries |
![]() |
|
Figure 14-16d Nuclear Protection [view large image] |
flying debris by the action of the blast. |