Monitoring Space Weather with a System of Ground-Based Cosmic Ray Detectors

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发表日期：

2024年2月1日

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V. V. Borog,
A. N. Dmitrieva,
Y. N. Mishutina

摘要

Abstract

Flicker noise spectroscopy is developed for the remote identification of processes of powerful solar activity in the form of coronal mass ejections (CMEs) directed toward the Earth. Results are presented from analyzing geo-effective events (>G1) using data from the international network of neutron monitors and the URAGAN multidirectional muon hodoscope that indicate the emergence of precursors (1–2 days in advance) of CMEs approaching the Earth’s orbit.