| Autor: |
Sheeley, N., Harvey, J., Feldman, W. |
| Zdroj: |
Solar Physics; Aug1976, Vol. 49 Issue 2, p271-278, 8p |
| Abstrakt: |
Observations of coronal holes, solar wind streams, and geomagnetic disturbances during 1973-1976 are compared in a 27-day pictorial format which shows their long-term evolution. The results leave little doubt that coronal holes are related to the high-speed streams and their associated recurrent geomagnetic disturbances. In particular, these observations strongly support the hypothesis that coronal holes are the solar origin of the high-speed streams observed in the solar wind near the ecliptic plane. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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