一、氦气测量发展简介早就知道,铀钍系列放射性元素衰变产生的α粒子,结合周围介质中的自由电子形成氦。这是地球氦(不考虑原始星球氦)生成的主要机理。人们自然地想到利用氦作为指示标志寻找铀矿。可是,由于种种技术上的原因,第一批有关铀矿床上样品中氦的分析数据迟至五十年代后期才发表。1957年,S.H.U.鲍威在南非维特瓦特斯兰德含铀金矿,收集了从山地工程中的断层和 First, the development of helium measurement Introduction It has long been known that the uranium-thorium series of radioactive elements decay of alpha particles, combined with the surrounding medium free electrons to form helium. This is the main mechanism by which Earth’s helium (regardless of the original planet’s helium) is generated. People naturally think of using helium as an indicator to look for uranium. However, due to various technical reasons, the first data on the analysis of helium in samples from uranium deposits were not published until later in the 1950s. In 1957, S.H.U. Bowei hosted a uranium-bearing gold deposit in Wirthurst, South Africa, collecting faults from mountainous works and