| Autor: |
Borog, V. V., Dmitrieva, A. N., Mishutina, Y. N. |
| Zdroj: |
Bulletin of the Russian Academy of Sciences: Physics; Feb2024, Vol. 88 Issue 2, p260-264, 5p |
| Abstrakt: |
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. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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