Transit of Sun Across Constellation Sagittarius and Variation of Secondary Gamma Radiation Flux in January, 2021 at Udaipur, India

P. Purohit, D. Pareek
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Abstract

We experimentally observed the variation of secondary gamma radiation flux (SGR) at Udaipur (27° 43’ 12.00” N, 75° 28’ 48.01” E), Rajasthan, India during transit of Sun across constellation Sagittarius in month of January, 2021. In this experimental study we used ground based NaI (Tl) Scintillation detector. Cadences of data were collected at interval of half an hour. The data files were stored in computer for half hour duration around time 17.00 IST to 17.30 IST on January 8, 9, 11, 13, 14, 17 and 18. The objective in this study is to observe secondary gamma radiation flux during transit of the Sun across the constellation Sagittarius. Analyzed data reveal significant variation of secondary gamma radiation flux (SGR). We interpret such variation of SGR flux counts on the basis of combine gravitational lensing effect due to Sun and Sagittarius constellation on background radiation, gravitational pull effect by constellation and sun on background radiation and radiation from constellation Sagittarius.
2021年1月印度乌代普尔太阳穿越人马座和二次伽马辐射通量的变化
本文于2021年1月在印度拉贾斯坦邦乌代浦尔(27°43 ' 12.00 " N, 75°28 ' 48.01 " E)对太阳经过人马座期间的二次伽马辐射通量(SGR)进行了观测。在本实验研究中,我们使用地基NaI (Tl)闪烁探测器。每隔半小时收集一次数据的节奏。数据文件在1月8日、9日、11日、13日、14日、17日和18日下午17:00至17:30左右在计算机中存储半小时。这项研究的目的是观察太阳在人马座凌日时的二次伽马辐射通量。分析数据显示二次伽马辐射通量(SGR)变化显著。我们基于太阳和人马座对背景辐射的联合引力透镜效应、星座和太阳对背景辐射的引力拉动效应以及人马座的辐射来解释SGR通量计数的变化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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