On the Reproduction of the Solar Activity Variations in the Range 2–40 Months in the Interplanetary Medium.
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| Title: | On the Reproduction of the Solar Activity Variations in the Range 2–40 Months in the Interplanetary Medium. |
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| Authors: | Bazilevskaya, G. A.1 (AUTHOR) bazilevskayaga@lebedev.ru, Kalinin, M. S.1 (AUTHOR), Krainev, M. B.1 (AUTHOR), Makhmutov, V. S.1 (AUTHOR), Svirzhevskaya, A. K.1 (AUTHOR), Svirzhevsky, N. S.1 (AUTHOR), Stozhkov, Yu. I.1 (AUTHOR) |
| Source: | Journal of Experimental & Theoretical Physics. Apr2022, Vol. 134 Issue 4, p479-486. 8p. |
| Subjects: | Interplanetary medium, Solar activity, Interplanetary magnetic fields, Solar oscillations, Galactic magnetic fields, Solar magnetic fields |
| Abstract: | We compare the quasi-biennial variations and Rieger-type variations (on a timescale of less than 1 year) in solar activity, interplanetary magnetic field, and galactic cosmic-ray flux modulation. We show that, in comparison with the 11-year cycle, the quasi-biennial variations are less suppressed in the interplanetary medium than on the Sun. Although the Rieger-type variations are adjacent in frequency to the quasi-biennial variations, they differ noticeably from them in the degree of reproduction in the interplanetary medium and the influence on the cosmic-ray modulation. [ABSTRACT FROM AUTHOR] |
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| Database: | Engineering Source |
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| Abstract: | We compare the quasi-biennial variations and Rieger-type variations (on a timescale of less than 1 year) in solar activity, interplanetary magnetic field, and galactic cosmic-ray flux modulation. We show that, in comparison with the 11-year cycle, the quasi-biennial variations are less suppressed in the interplanetary medium than on the Sun. Although the Rieger-type variations are adjacent in frequency to the quasi-biennial variations, they differ noticeably from them in the degree of reproduction in the interplanetary medium and the influence on the cosmic-ray modulation. [ABSTRACT FROM AUTHOR] |
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| ISSN: | 10637761 |
| DOI: | 10.1134/S1063776122040021 |
