The muon charge asymmetry and the directional distribution of thunderstorm events observed by the GRAPES-3 muon telescope

IF 6.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
B. Hariharan,S.K. Gupta,Y. Hayashi,P. Jagadeesan,A. Jain,S. Kawakami,H. Kojima,P.K. Mohanty,Y. Muraki,P.K. Nayak,A. Oshima,M. Rameez,K. Ramesh,L.V. Reddy,S. Shibata
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Abstract

Abstract The intense electric fields inside thunderstorms can significantly modify the intensity of secondary cosmic ray muons at the ground level, producing measurable variations in their intensity (|ΔI μ | >0.3%). By utilizing the decade-long observations of thunderstorms (April 2011–December 2020) by the GRAPES-3 muon telescope (G3MT), a directional asymmetry in |ΔI μ | is observed, with nearly six times more events being detected from the east than the west directions. Using detailed CORSIKA Monte Carlo simulations, we present that this asymmetry is caused by the variations of the muon charge ratio R μ (N μ + /N μ - ). The anisotropic R μ in turn, is caused by the systematic changes in geomagnetic effects, and subsequent selective filtering of predominantly positively charged primary cosmic rays. As a consequence, the R μ increases systematically from west to east across the G3MT field of view, enhancing the sensitivity of east directions to charged thunderstorms. Independent meteorological validation using ground-based electric field mill data confirms that the thunderstorm trajectories exhibit no eastward preference, ruling out localized storm clustering as a source of the asymmetry. Monte Carlo simulations with constant R μ show that the directional asymmetry disappears, indicating the muon charge imbalance to be the dominant driver of the observed asymmetry. Furthermore, we evaluated the systematic robustness of the framework against variations in hadronic interaction generators, thundercloud configuration, and |ΔI μ |. The dependence of R μ on the hadronic interaction is studied extensively by comparing seven combinations of high-, and low-energy hadronic interaction generators, which show a ≲7% spread in R μ , and ≲14% variation in the derived thunderstorm potentials. These results provide the first quantitative link between the muon charge asymmetry caused by the geomagnetic field, and the directional distribution of thunderstorms, reinforcing the role of muon observations as a probe of gigavolt potentials in atmospheric electrical structures.
GRAPES-3 μ子望远镜观测到的雷暴事件的μ子电荷不对称性和方向分布
雷暴内部的强电场可以显著改变次级宇宙射线μ介子在地面的强度,产生可测量的强度变化(|ΔI μ | >0.3%)。利用GRAPES-3 μ介子望远镜(G3MT)长达十年的雷暴观测(2011年4月至2020年12月),观测到|ΔI μ |的方向不对称,从东方向探测到的事件几乎是从西方向探测到的事件的六倍。通过CORSIKA蒙特卡罗模拟,我们发现这种不对称性是由介子电荷比R μ (N μ + /N μ -)的变化引起的。而各向异性R μ则是由地磁效应的系统变化和随后对主要带正电的初级宇宙射线的选择性过滤引起的。因此,整个G3MT视场的R μ从西向东有系统地增大,增强了东部方向对带电雷暴的敏感性。利用地面电场磨数据进行的独立气象验证证实,雷暴轨迹没有表现出向东的偏好,排除了局部风暴聚集作为不对称来源的可能性。常数R μ的蒙特卡罗模拟表明,方向不对称性消失,表明介子电荷不平衡是观察到的不对称性的主要驱动因素。此外,我们评估了该框架对强子相互作用发生器、雷云结构和|ΔI μ |变化的系统鲁棒性。通过比较高能和低能强子相互作用发生器的7种组合,研究了R μ对强子相互作用的依赖关系,它们在R μ上的分布为> 7%,推导出的雷暴势的变化为> 14%。这些结果首次提供了由地磁场引起的μ子电荷不对称与雷暴定向分布之间的定量联系,加强了μ子观测作为大气电结构中千伏电位探测的作用。
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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