Characteristics of recurrent Forbush decreases in Galactic cosmic ray intensity during positive and negative solar magnetic polarities
Author:
Funder
Mahasarakham University
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s10509-021-03970-2.pdf
Reference31 articles.
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2. Badruddin, Kumar, A.: Sol. Phys. 291(2), 559 (2016). https://doi.org/10.1007/s11207-015-0843-4
3. Barouch, E., Burlaga, L.F.: J. Geophys. Res. 80(4), 449 (1975). https://doi.org/10.1029/JA080i004p00449
4. Barouch, E., Burlaga, L.F.: J. Geophys. Res. 81(13), 2103 (1976). https://doi.org/10.1029/JA081i013p02103
5. Belov, A.V.: In: Gopalswamy, N., Webb, D.F. (eds.) Universal Heliophysical Processes, vol. 257, p. 439 (2009). https://doi.org/10.1017/S1743921309029676
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