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作 者:易惟熙 沈承德 王道德 O.EUGSTER J.BEER M.SUTER W.WOLFLI
机构地区:[1]Institute of Geochemistry,Academia Sinica,Guiyang [2]Physikalisches Institut,Universitt Bern,Switzerland [3]Institut für Mittelenergiephysik,ETH Zürich,Switzerland
出 处:《Chinese Science Bulletin》1989年第5期426-430,共5页
摘 要:<sup>10</sup>Be is mainly produced in meteorite by spallation reactions of cosmic ray particles with oxygen, magnesium, silicon or nitrogen in it. The threshold energy is above 500 MeV. The half lifetime of <sup>10</sup>Be in between <sup>26</sup>Al and <sup>53</sup>Mn is 1.6 Ma. Thus the possibility of routine determination of <sup>10</sup>Be in a large number of meteorites constitutes an improvement in studying the exposure conditions of
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