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Observation of the Track-Pit Swarms in the Plastic Track Detectors exposed in Space

机译:在暴露于太空的塑料轨道探测器中观察轨道坑群

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@@ For further check of the pit nature Erzionhypothesis [1] it has been executed the precise, at high1200-multiple magnification in optical microscopeattendance of a large square in the Plastic Solid-StateTrack Detectors (PSSTD), which were satellite exposedin Space [2]. It was analyzed films of PSSTD CR-39 andCN-85 from different piles and satellite flights. By thismanner on the total of searched PSSTD surface about 20cm 2 have been primarily discovered a range of thespecific, compact pit groups, characteristics for whichindicate that their source are the swarms of the not-knowingorigin particles in the track-detector matter.
机译:@@为了进一步检查凹坑性质Erzionhypothesis [1],已执行了精确的光学显微镜放大倍数为1200倍的塑料固态轨道检测器(PSSTD)中的大正方形的定标,这些定标被暴露在太空中[2] ]。分析了来自不同桩和卫星飞行的PSSTD CR-39和CN-85的电影。通过这种方式,在大约20cm 2的被搜索PSSTD表面总数上,主要发现了一系列特定的致密凹坑组,这些特征表明它们的来源是轨迹检测器物质中不知道来源的粒子群。

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  • 会议地点 Beijing(CN)
  • 作者单位

    Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Science, 119991, Kosygin str. 19,Moscow;

    Pushkov Terrestrial Magnetism, Ionosphere and Radiowave Propagation Institute, Russian Academy of Science,Troitsk, Moscow region;

    Lomonosov Moscow State University, Chemical Department, Radiochemical Division, Moscow;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 宇宙射线强度变化;
  • 关键词

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