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Preferred bartels days of high-speed plasma streams in the solar wind

✍ Scribed by B. A. Lindblad


Publisher
Springer
Year
1981
Tongue
English
Weight
406 KB
Volume
74
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES


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

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Interplanetary magnetic field data compiled by King (1977King ( , 1979) ) are used to obtain a list of high velocity solar wind streams for the period January 1975 through June 1978. The catalogue is a continuation of a previous list which covered 1964-75. The total number of high-speed solar wind s

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Interplanetary magnetic field data obtained from near-Earth spacecraft are used to compile a catalogue of high-velocity solar wind streams for the period June 1978 through October 1982 (Barrels rotations 1980(Barrels rotations -2039)). The compilation of high-velocity streams is a continuation of tw