2023 年 11 月 5 日日冕扰动导致地基宇宙射线探测器计数率增加

A. Chilingarian, T. Karapetyan, B. Sargsyan, M. Zazyan, Johannes Knapp, Michael Walter, T. Rehm
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引用次数: 0

摘要

这封信介绍了一种与太阳活动有关的罕见物理现象,表现为大气中的中子、电子和伽马射线通量异常。通常,地球磁场干扰会降低到达地表的宇宙射线强度。然而,宇宙射线通量会间歇性地出现暂时性激增,这被称为磁层效应(ME)。我们的观测发现,这种效应主要会导致位于中纬度山顶的粒子探测器的计数率上升。2023 年 11 月 5 日,位于山顶的中子监测器的计数率增加了 2-3%,记录电子和伽马射线的薄塑料闪烁器的计数率增加了 5%。通量的增加与行星际磁场的南移相吻合。重要的是,我们首次展示了在两个山顶观测到的磁层效应能谱:阿拉加茨和祖格峰。对地球大气中低能质子相互作用的模拟证实了低能宇宙射线的增强作用。质子通常受到地磁截止的限制,但却进入了地球大气层,在地球表面产生了可探测到的粒子群。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Increase in the count rates of ground-based cosmic-ray detectors caused by the heliomagnetic disturbance on 5 November 2023
This letter presents a rare physical phenomenon associated with solar activity, manifesting in anomalies within neutron, electron, and gamma-ray fluxes in the atmosphere. Conventionally, Earth's magnetic field disturbances reduce cosmic ray intensity reaching the surface. However, a temporary surge in cosmic ray flux occurs intermittently known as the Magnetospheric Effect (ME). Our observations reveal that this effect predominantly induces a count rate increase in particle detectors positioned at middle latitudes on mountaintops. On November 5, 2023, a 2-3% increase in neutron monitors at mountain altitudes and up to 5% increase in thin plastic scintillators registering electrons and gamma rays. This flux escalation coincided with a southward orientation of the interplanetary magnetic field. Importantly, we present, for the first time, the energy spectrum of the Magnetospheric Effect observed at two mountaintops: Aragats and Zugspitze. Simulations of low-energy proton interactions in the terrestrial atmosphere affirm the augmentation of low-energy cosmic rays. Protons, typically restricted by the geomagnetic cutoff, reached the Earth's atmosphere, generating detectable particle showers on the Earth's surface.
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