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

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 neutro...

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Bibliographic Details
Published in:Bulletin of the Russian Academy of Sciences. Physics 2024-02, Vol.88 (2), p.260-264
Main Authors: Borog, V. V., Dmitrieva, A. N., Mishutina, Y. N.
Format: Article
Language:English
Subjects:
Coronal mass ejection
Cosmic rays
Hadrons
Heavy Ions
Nuclear Physics
Physics
Physics and Astronomy
Solar activity
Solar corona
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Summary: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.
ISSN:1062-8738
1934-9432
DOI:10.1134/S1062873823705342