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SOURCES OF RADIATION - RCT STUDY GUIDE - NukeWorker.com

SOURCES OF RADIATION - RCT STUDY GUIDE - NukeWorker.com

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1.05 - <strong>SOURCES</strong> <strong>OF</strong> <strong>RADIATION</strong> <strong>RCT</strong> <strong>STUDY</strong> <strong>GUIDE</strong>background should be greatly reduced. The use of balloons carrying ion chambers togreat heights yielded data which showed the effect increased, rather than decreased.These and other data showed that radiation was really <strong>com</strong>ing from outer space. Thename cosmic rays was given to this high energy.Further study has shown that cosmic radiation consists of two parts: primary andsecondary. The primary <strong>com</strong>ponent may be further divided into galactic, geomagneticallytrapped radiation, and solar.PrimaryThe galactic cosmic rays <strong>com</strong>e from outside the solar system and are <strong>com</strong>posedmostly of positively charged particles. Studies have shown that outside the earth'satmosphere, cosmic rays consist of 87% protons, of 11% alpha particles, andabout 1% each of other heavier nuclei and electrons at latitudes above 55 degrees.These particles may have energies in the range of about 1 GeV and higher.As a charged particle approaches the earth, it is acted upon by the earth's magneticfield. In order to pass on through to the earth, the particle must have a certainmomentum. Otherwise, it may be trapped by the earth's magnetic field. This givesrise to the second type of primary cosmic rays, the geomagnetically trappedradiation.Solar cosmic rays are produced following severe solar flares on the surface of thesun. These rays consist of protons. The events are classed as high energy or lowenergy. The high energy events can be observed by ground-level neutron devices.The low energy events are more frequent but must be detected at high altitude.Since these events produce radiation throughout the solar system, they are of greatimportance in shielding design for manned space missions.SecondarySecondary cosmic rays result from interactions which occur when the primary raysreach the earth's atmosphere. When the high energy particles collide with atoms ofthe atmosphere, many products are emitted: pions, muons, electrons, photons,protons, and neutrons. These, in turn, produce other secondaries as they collidewith elements or decay on the way toward the earth's surface. Thus, a8multiplication or shower occurs in which as many as 10 secondaries may resultfrom a single primary.-4- Issued 05/95

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