Cosmic ray fluctuations and MHD waves in the solar wind
During large-scale solar wind disturbances, variations in galactic cosmic rays with periods from several minutes to 2–3 hours, which are called cosmic ray fluctuations in the scientific literature, often occur. Such fluctuations are not observed in the absence of disturbances. Since cosmic rays are...
| Main Authors: | Starodubtsev S. A., Zverev A. S., Gololobov P. Y., Grigoryev V. G. |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
INFRA-M
2023-06-01
|
| Series: | Solar-Terrestrial Physics |
| Subjects: | |
| Online Access: | https://naukaru.ru/en/nauka/article/57383/view |
Similar Items
-
MHD waves at the pre-front of interplanetary shocks on September 6 and 7, 2017
by: Starodubtsev S. A., et al.
Published: (2024-09-01) -
Impact of solar magnetic field amplitude and geometry on cosmic rays diffusion coefficients in the inner heliosphere
by: Perri Barbara, et al.
Published: (2020-01-01) -
Effects of anomalous cosmic rays on the solar wind events in the outer heliosphere
by: Yucheng Zhou, et al.
Published: (2024-02-01) -
Transport of Cosmic-Ray Electrons from 1 au to the Sun
by: Vahé Petrosian, et al.
Published: (2023-01-01) -
PECULIARITIES OF SPORADIC VARIATIONS IN DENSITY AND ANISOTROPY OF GALACTIC COSMIC RAYS IN SOLAR CYCLE 24
by: V.G. Grigoryev, et al.
Published: (2022-03-01)