Similarities and Differences between Forbush Decreases Associated with Streams from Coronal Holes, Filament Ejections, and Ejections from Active Regions-Reference-Cited by-同舟云学术

Similarities and Differences between Forbush Decreases Associated with Streams from Coronal Holes, Filament Ejections, and Ejections from Active Regions

Published:2022-06 Issue:3 Volume:62 Page:159-177
ISSN:0016-7932
Container-title:Geomagnetism and Aeronomy
language:en
Short-container-title:Geomagn. Aeron.

Author:

Melkumyan A. A.,Belov A. V.,Abunina M. A.,Shlyk N. C.,Abunin A. A.,Oleneva V. A.,Yanke V. G.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Geophysics

Link

https://link.springer.com/content/pdf/10.1134/S0016793222030112.pdf

Reference48 articles.

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2. Abunina, M.A., Belov, A.V., Shlyk, N.S., Eroshenko, E.A., Abunin, A.A., Oleneva, V.A., Pryamushkina, I.I., and Yanke, V.G., Forbush effects created by coronal mass ejections with magnetic clouds, Geomagn. Aeron. (Engl. Transl.), 2021, vol. 61, no. 5, pp. 678–687.

3. Badruddin, Yadav, R.S., and Yadav, N.R., Influence of magnetic clouds on cosmic-ray intensity variation, Sol. Phys., 1986, vol. 105, no. 5, pp. 413–428.

4. Belov, A.V., Forbush effects and their connection with solar, interplanetary and geomagnetic phenomena, Proc. IAU Symp., 2009, no. 257, pp. 119–130.

5. Belov, A.V., Eroshenko, E.A., Oleneva, V.A., Struminsky, A.B., and Yanke, V.G., What determines the magnitude of Forbush decreases?, Adv. Space Res., 2001, vol. 27, no. 3, pp. 625–630. https://doi.org/10.1016/S0273-1177(01)00095-3

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