Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976
- 1 August 1976
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 49 (2) , 271-278
- https://doi.org/10.1007/bf00162451
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
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- Solar rotation as marked by extreme-ultraviolet coronal holesThe Astrophysical Journal, 1975
- Solar coronal holes as sources of recurrent geomagnetic disturbancesJournal of Geophysical Research, 1974
- Observation of sectored structure in the outer solar corona: Correlation with interplanetary magnetic fieldSolar Physics, 1974
- A coronal hole and its identification as the source of a high velocity solar wind streamSolar Physics, 1973
- Measurements of the interplanetary solar wind during the large geomagnetic storm of April 17-18, 1965Journal of Geophysical Research, 1967
- The solar wind velocity and its correlation with cosmic-ray variations and with solar and geomagnetic activityJournal of Geophysical Research, 1963