Preferred Bartels days of high speed solar wind streams: an update

Preferred Bartels days of high speed solar wind streams: an update

Comparison of the distribution of solar wind streams as a function of Bartels rotation days for two successive epochs indicates several significant differences. These may be due to the differing nature of IMF and solar wind in solar cycles 20 and 21.

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Bibliographische Detailangaben
Veröffentlicht in:Solar physics 1989-01, Vol.122 (1), p.187-189
Hauptverfasser: RANGARAJAN, G. K, MAVROMICHALAKI, H
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Earth, ocean, space
Exact sciences and technology
Interplanetary space
Solar system
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Beschreibung
Zusammenfassung:Comparison of the distribution of solar wind streams as a function of Bartels rotation days for two successive epochs indicates several significant differences. These may be due to the differing nature of IMF and solar wind in solar cycles 20 and 21.
ISSN:0038-0938
1573-093X
DOI:10.1007/BF00162834