TM 5-6635-386-12&Pbackscatter operations and permit simultaneouscounting of both density and moisture.Approximately 90% of the moisture count is obtainedfrom returned thermal neutrons from the closest 6 inchesof soil.1-3. PRINCIPLES OF OPERATIONGeneralVarious elements, both naturally occurring (Radium) andreactor produced (Cesium and Americium) are unstableand are slowly decaying to a more stable state. The actof decay produces emissions of energy upondisintegration of the atoms.These emissions are either "rays" of electromagneticradiation (Gamma Rays) or are actual particles ofmaterial (neutrons, for example). Other emissions areproduced from various radioactive materials; however,we are concerned with only the gamma and neutronradiation for purposes of nuclear soil testing.Gamma radiation is emitted in several energy levels by asealed Radium source and in a single energy level by aCesium source. The Cesium level is 0.66 MEV andrequires less shielding than the multi-level output of theRadium source. The fixed spectrum emission is alsosuperior for soil density determination purposes.Cesium, a reactor produced isotope requires a licensefor use anywhere in the U.S. and in foreign countries.Neutron emission occurs when an alpha particle emitter(Americium, Plutonium, or Radium) is mixed withBeryllium powder in a tightly compressed pellet. Thealpha particles strike the Beryllium atoms to produce fastneutrons of an average energy of 5 million electron volts.The suffix "Be" is attached to the alpha source name todenote its use as a neutron source when it is mixed withBeryllium (RaBe, AmBe, PuBe).These emissions are detected by appropriate detectors(Geiger Mueller tubes) for gamma and (Boron Tri-fluoride-BF3 or Helium-3 H3 tubes) neutronmeasurements. The resultant signals are displayedelectronically as an index of soil density and moisture.Radioactivity, both gamma and neutron, may be thoughtof as being similar to light from an incandescent bulb.The light rays diminish rapidly as we move away from thebulb (by the inverse square of the distance from thelamp), and they have the ability to penetrate variousmaterials to some degree, ranging from nearly completepenetration (glass) to nearly complete blockage (metalshield).Radiation obeys the same rules, although its penetrationcapabilities are generally much greater than light. Thefarther we are from the source, the safer we are, and themore absorbing material (shielding) we place betweenourselves and the source, the safer we are. It istheoretically impossible to shield any radioactive sourcecompletely; however, careful tester design andappropriate choice of shielding materials can reduce theradiation to an acceptable level with negligible absorptionby the user under proper operating procedures.Gamma RadiationGamma radiation is electromagnetic "photon" energycapable of penetration of several inches of mostmaterials. It is essentially high energy "light ray" energy.It is useful for the total mass measurement of heavymaterials and is used to determine total density of soil.Neutron RadiationNeutron radiation consists of small, noncharged particlesemitted from the source at an average energy level ofapproximately 5.0 MEV. This is known as "fast" neutronemission. Neutron detectors "see" only slow, or"’thermal" neutrons. Therefore, the fast neutrons mustslow down or they will be ignored by the detectors.Neutrons slow down by colliding with other objects muchlike a rifle bullet ricocheting from rock to rock.Collision of the fast neutrons with the nuclei of largeatoms results in rebounding of the neutrons with littleloss of energy. Collision with the orbiting electrons(approximately 1/1840th the weight of a neutron)produces little loss of energy. However, collision with an1-3
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