吉林陨石钻孔样品中宇宙线成因核素的深度分布与宇宙线照射历史

成功地对吉林Ⅰ号陨石取得了平行与垂直第一阶段母体表面并相交于第二阶段母体中心的钻孔岩蕊.对两个钻孔的样品进行了系统的宇宙线成因核素(³He,^20,21,22Ne,²²Na,²⁶Al,⁵³Mn,⁶⁰Co)、放射成因气体和俘捕稀有气体的研究,证实吉林陨石具有典型的两阶段宇宙线照射历史,确证作者曾提出的两阶段母体年龄、形状、大小及各样品埋藏位置的模式是合理的.各样品散裂、放射和俘捕气体的研究表明:气体的丢失机制是第二阶段母体在行星际空间运行时受到太阳的周期性加热.根据Ⅱ号陨石各定位样品的^3,4He,^20,21,22Ne和⁴⁰Ar的研究,恢复了Ⅱ号陨石在两阶段母体中的相对位置.     

南极岩石样品中稀土元素的中子活化分析

用仪器中子活化分析技术,测定了南极岩石中8种稀土元素含量,讨论了不同岩石的稀土模式特点。     

A STUDY ON ~(10)Be IN QUARTZ FROM LOESS OF CHINA (Ⅰ)——In situ COSMOGENIC ~(10)Be AND EROSION RATES OF SOURCE REGIONS OF LOESS

In situ cosmogenic ~(10)Be in quartz from loess deposited in the last 2,000,000 a is considered to have been derived mainly from initial ~(10)Be in source regions and it bears abundant information about changes in erosion rates of source regions. As [have been estimated, the concentrations of "in situ cosmogenic ~(10)Be" in quartz from samples GL47(L1) andGL83 (L2) collected from the Luochuan loess section are 5×10~5 atom/g and 2.2×10~6 atom/g, respectively. As calculated on the basis of the above estimates, the erosion rates of the source regions are: εBeL1=1.5×10~(-3) cm/a for the L1 period (10,000—90,000 a) and εBeL2=3.8×10~(-4) cm/a for the L2 period (130,000—190,000 a). Studies of "in situ cosmogeuic ~(10)Be" in quartz from loess at deeper levels are expected to be applied to ~(10)Be dating of loess strata.     

中国黄土石英中的~(10)Be研究——Ⅰ.“自身成因~(10)Be”与黄土源区侵蚀速率

对于0.2Ma以来的黄土堆积物,其石英“自身成因~(10)Be”主要来源于源区初始~(10)Be,载带着源区侵蚀速率变化信息。中国洛川黄土剖面GL 47(L_1),GL83(L_2)两样品石英“自身成因~(10)Be”浓度分别为5×10~5原子/g,2.2×10~6原子/g。据此计算的源区侵蚀速率为:L_1期(10—90ka),ε_(BeL_1)=1.5×10~(-3)cm/a;L_2期(130—190k a),ε_(BeL_2)=3.8×10~(-4)cm/a。更深层位黄土石英“自身成因~(10)Be”研究可望用于黄土地层测年。