Rigidity Spectrum of Forbush Effects Observed During Solar Cycles 24 and 25
The work presents an analysis of the rigidity spectrum of Forbush decreases observed over 24–25 Solar Cycles. The URAGAN muon hodoscope and Moscow neutron monitor data were used as information on cosmic ray variations. To determine the rigidity spectrum of Forbush decreases, the median rigidity method was utilized. The dependence of the spectrum index on the phase of solar activity and the polarity of the general magnetic field of the Sun is discussed.
Authors
- И. И. Астапов (ORCID: https://orcid.org/0000-0002-6746-3910)
- N. S. Barbashina (ORCID: https://orcid.org/0000-0001-5215-4296)
- I. A. Lagoida (ORCID: https://orcid.org/0000-0002-2664-6550)
- P. S. Kuzmenkova
- В. В. Шутенко (ORCID: https://orcid.org/0000-0003-4102-2989)
- Yu. N. Mishutina
- Polina Sukhova
Institutions
- National Research Nuclear University MEPhI (RU)
Publication Details
- Journal
- Physics of Atomic Nuclei
- Published
- 2024-12-01
- DOI
- https://doi.org/10.1134/s1063778824110085
- Citations
- 2
- Primary Topic
- Solar and Space Plasma Dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.66