Recurrent and sporadic Forbush decreases during solar cycles 23–24
A comparison has been made between recurrent (associated with high-speed streams from coronal holes) and sporadic (caused by interplanetary coronal mass ejections (ICMEs)) Forbush decreases (FDs) in solar cycles 23 and 24 (as well as in the maxima of these cycles and the minimum between them). Forbu...
Main Authors: | Melkumyan A.A., Belov A.V., Abunina M.A., Abunin A.A., Eroshenko E.A., Oleneva V.A., Yanke V.G. |
---|---|
Format: | Article |
Language: | English |
Published: |
INFRA-M
2019-03-01
|
Series: | Solar-Terrestrial Physics |
Subjects: | |
Online Access: | https://naukaru.ru/en/nauka/article/28040/view |
Similar Items
-
The interaction of the galactic cosmic rays with the high-speed solar wind streams
by: A. I. Klyuyeva
Published: (2014-12-01) -
Investigating tensor anisotropy of cosmic rays during large-scale solar wind disturbances
by: Gololobov P.Yu., et al.
Published: (2017-06-01) -
Editorial: Magnetic Flux Ropes: From the Sun to the Earth and Beyond
by: Rui Liu, et al.
Published: (2020-11-01) -
Influence of coronal mass ejections on parameters of high-speed solar wind: a case study
by: Shugay Yulia, et al.
Published: (2018-01-01) -
Near-earth solar wind flows and related geomagnetic activity during more than four solar cycles (1963–2011)
by: Richardson Ian G., et al.
Published: (2012-05-01)