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Management of Commercially Generated Radioactive Waste - U.S. ...

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3.3.1.1 Cosmic Radiation<br />

3.27<br />

Cosmic radiation refers both to primary energetic particles <strong>of</strong> extraterrestrial origin<br />

that strike the earth's atmosphere and to secondary particles generated by the interaction<br />

<strong>of</strong> primary particles with the atmosphere (radionuclides produced by cosmic radiation are<br />

discussed later). The primary cosmic radiation consists <strong>of</strong> particles produced outside the<br />

solar system and particles emitted by the sun. The cosmic ray dose rate to the population<br />

living at sea level is about 26 mrem per year, taking into account shielding from struc-<br />

tures. Considering the altitude distribution <strong>of</strong> the U.S. population, the average dose rate<br />

is 28 mrem per year. In Denver, which is the largest city at a relatively high altitude<br />

(1600 meters) in the United States, the average dose rate from cosmic rays is about 50 mrem<br />

per year. In Leadville, Colorado (3200 meters), which has a population <strong>of</strong> about 10,000,<br />

the average cosmic ray dose rate amounts to 125 mrem per year. High altitude airplane<br />

flights add a small fraction to the population dose from cosmic rays at ground level. For<br />

example, a jet flight <strong>of</strong> 5 hours duration (e.g., transcontinental or transatlantic at 12 km<br />

altitude) at mid-latitudes would result in a dose <strong>of</strong> approximately 2.5 mrem to the whole<br />

body. An extreme case would be a 10-hr polar route flight from, for example, California to<br />

Europe where the long flight time and the higher cosmic ray intensities at high latitudes<br />

would result in a passenger dose <strong>of</strong> approximately 10 mrem (or 20 mrem for a round trip).<br />

3.3.1.2 Terrestrial Radioactivity<br />

Terrestrial radioactive material is present in the environment because naturally<br />

radioactive isotopes are constituents <strong>of</strong> a number <strong>of</strong> elements in the earth's crust. The<br />

nuclear interaction <strong>of</strong> cosmic rays with constituents <strong>of</strong> the atmosphere, soil, and water<br />

also produce a number <strong>of</strong> different radionuclides. These naturally occurring radionuclides<br />

give rise to both external and internal irradiation <strong>of</strong> man.<br />

Cosmogenic Radionuclides<br />

Cosmogenic radionuclides are produced through interaction <strong>of</strong> cosmic rays with atoms in<br />

the atmosphere and in the outermost layer <strong>of</strong> the earth's crust. The entire geosphere con-<br />

tains radionuclides produced in this fashion. The four cosmogenic radionuclides that con-<br />

3 7<br />

tribute measurable dose to man are hydrogen-3 (tritium) ( H), beryllium-7 ( Be), carbon-14<br />

(14C), and sodium-22 (22Na), all produced in the atmosphere. The total contribution to<br />

the average dose rate (in addition to direct cosmic radiation) by these four nuclides is<br />

less than 1 mrem/yr.<br />

Primordial Radionuclides<br />

Several dozen naturally occurring nuclides are radioactive with half-lives <strong>of</strong> at least<br />

the same order <strong>of</strong> magnitude as the estimated age <strong>of</strong> the earth (4.5 x 10 9 yr), and are con-<br />

sequently assumed to represent a primordial inventory (that is, some radionuclides are<br />

remaining since the formation <strong>of</strong> the world). There are three chains or series radionu-<br />

clides headed by thorium-232 (232Th), uranium-235 (235U), and uranium-238 ( 238 U). These<br />

radionuclides decay ultimately to a stable isotope <strong>of</strong> lead through a chain <strong>of</strong> decaying<br />

nuclides <strong>of</strong> wide ranging half-lives. These chains contain the, perhaps more familiar,

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