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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| Veröffentlicht in: | Solar physics 1989-01, Vol.122 (1), p.187-189 |
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| container_end_page | 189 |
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| container_issue | 1 |
| container_start_page | 187 |
| container_title | Solar physics |
| container_volume | 122 |
| creator | RANGARAJAN, G. K MAVROMICHALAKI, H |
| description | 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. |
| doi_str_mv | 10.1007/BF00162834 |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 0038-0938 |
| ispartof | Solar physics, 1989-01, Vol.122 (1), p.187-189 |
| issn | 0038-0938 1573-093X |
| language | eng |
| recordid | cdi_proquest_miscellaneous_18282139 |
| source | SpringerLink Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
| subjects | Astronomy Earth, ocean, space Exact sciences and technology Interplanetary space Solar system |
| title | Preferred Bartels days of high speed solar wind streams: an update |
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