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.
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]
Copyright of Journal of Experimental & Theoretical Physics is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: On the Reproduction of the Solar Activity Variations in the Range 2–40 Months in the Interplanetary Medium.
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  Data: <searchLink fieldCode="JN" term="%22Journal+of+Experimental+%26+Theoretical+Physics%22">Journal of Experimental & Theoretical Physics</searchLink>. Apr2022, Vol. 134 Issue 4, p479-486. 8p.
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  Data: <searchLink fieldCode="DE" term="%22Interplanetary+medium%22">Interplanetary medium</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+activity%22">Solar activity</searchLink><br /><searchLink fieldCode="DE" term="%22Interplanetary+magnetic+fields%22">Interplanetary magnetic fields</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+oscillations%22">Solar oscillations</searchLink><br /><searchLink fieldCode="DE" term="%22Galactic+magnetic+fields%22">Galactic magnetic fields</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+magnetic+fields%22">Solar magnetic fields</searchLink>
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  Label: Abstract
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  Data: 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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  Data: <i>Copyright of Journal of Experimental & Theoretical Physics is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1134/S1063776122040021
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      – SubjectFull: Interplanetary medium
        Type: general
      – SubjectFull: Solar activity
        Type: general
      – SubjectFull: Interplanetary magnetic fields
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      – SubjectFull: Solar oscillations
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      – SubjectFull: Galactic magnetic fields
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              Text: Apr2022
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