Variation of Secondary Gamma Radiation Flux during Closest Approach of Mars towards Earth, Mars at Opposition and Transit of Moon across Different Constellations and Planets in the Month of October, 2020 at Udaipur, India

IF 0.5 Q4 PHYSICS, MULTIDISCIPLINARY Jordan Journal of Physics Pub Date : 2022-10-31 DOI:10.47011/15.4.10
D. Pareek, Pallavi Sengar
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Abstract

Abstract: The experimental studies of closest approach of Mars towards Earth on October 6 & 7, 2020, Mars at opposition on October 13, 2020 and transit of Moon across different constellations and planets at Udaipur (270 43’ 12.00” N, 750 28’ 48.01” E), Rajasthan, India were conducted in the month of October, 2020 using a ground-based NaI (Tl) scintillation detector. For the closest approach of Mars, the data files were stored in computer for a half-hour duration from 20.30 IST to 1.00 IST on the dates of October 6 & 7, 2020, for Mars at opposition data files stored in computer for a half-hour duration from 18.00 IST to 20.00 IST on the date of October 13, 2020 and for Moon in the constellation experimental study the data files were stored in computer for a half-hour duration for the time 18.30 IST – 19.00 IST in the month of October, 2020 dated 19, 21, 22, 23, 25, 27, 28 and 29 at Udaipur (270 43’ 12.00” N, 750 28’ 48.01” E), Rajasthan, India, using a ground-based NaI (Tl) scintillation detector. For these experimental studies, the calibration of the scintillation detector was 2 keV per channel using a standard Cs137 source. Therefore, we detected the secondary radiation flux in the energy range from 2 keV to 2 MeV. Analyzed data of closest approach of Mars revealed a significant enhancement of secondary gamma-radiation flux (SGR) of about 4.5% on closest approach of Mars towards Earth at time 00.00 IST -00.30 IST (October 7) in comparison to the time 20.30 IST -21.00 IST (October 6). We interpret that such enhancement of SGR flux is on the basis of closest approach of Mars towards Earth, reflection of solar radiation from Mars towards Earth and gravitational lensing effect produced by Mars. For Mars at opposition, the analyzed data revealed a significant enhancement of secondary gamma-radiation flux (SGR) of about 1.7% in between times 19.00 IST – 19.30 IST. We interpret such enhancement of SGR flux on the basis of Mars at opposition, combined gravitational pull due to planet Mars, planet Earth and the Sun and gravitational lensing by Mars and for transit of Moon, the analyzed data revealed a significant variation of secondary gamma radiation flux (SGR) in the month of October. We interpret such variation of SGR flux on the basis of transit of Moon across different constellations and planets in the month of October. Keywords: Cosmic radiation, Reflection of solar radiation, Secondary gamma radiation, Closest approach of Mars, Mars at opposition, Combined gravitational pull and gravitational lensing effect by Mars, Transit of Moon across different constellations and planets.
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2020年10月在印度乌代普尔,火星最接近地球、火星冲日和月球穿越不同星座和行星时二次伽马辐射通量的变化
摘要:2020年10月,使用地面NaI(Tl)闪烁探测器,对火星于2020年10月份6日和7日最接近地球、火星于2020月13日处于对立面以及月球在印度拉贾斯坦邦乌代浦(270 43'12.00“N,750 28'48.01”E)不同星座和行星之间的凌日进行了实验研究。对于最接近火星的情况,数据文件存储在计算机中,持续时间为2020年10月6日和7日国际标准时间20.30至1.00,而火星在10月13日国际标准标准时间18.00至20.00,持续时间半小时,2020年和2020年10月19日、21日、22日、23日、25日、27日、28日和29日,在印度拉贾斯坦邦乌代浦(270 43'12.00“N,750 28'48.01”E),使用地面NaI(Tl)闪烁探测器,将数据文件存储在计算机中半小时,时间为18.30 IST–19.00 IST。对于这些实验研究,使用标准Cs137源对闪烁探测器的校准为每个通道2keV。因此,我们检测到了能量范围从2keV到2MeV的二次辐射通量。火星最近接近的分析数据显示,与国际标准时间20.30至国际标准时间-21.00(10月6日)相比,在国际标准时间00.00至0030(10月7日)火星最接近地球时,二次伽马辐射通量(SGR)显著增强约4.5%。我们认为,SGR通量的增强是基于火星离地球最近、火星太阳辐射对地球的反射以及火星产生的引力透镜效应。对于处于对立面的火星,分析数据显示,在19.00 IST至19.30 IST之间,二次伽马辐射通量(SGR)显著增强约1.7%。我们根据火星的相对位置、火星、地球和太阳的引力以及火星的引力透镜作用和月球凌日来解释SGR通量的增强,分析的数据揭示了10月份次级伽马辐射通量(SGR)的显著变化。我们根据10月份月球在不同星座和行星之间的凌日来解释SGR通量的这种变化。关键词:宇宙辐射、太阳辐射的反射、二次伽马辐射、火星最接近、火星相对、火星的引力拉和引力透镜效应,月球在不同星座和行星之间的凌日。
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来源期刊
Jordan Journal of Physics
Jordan Journal of Physics PHYSICS, MULTIDISCIPLINARY-
CiteScore
0.90
自引率
14.30%
发文量
38
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