Geomagnetic Disturbances Around the Solar Minimum of Cycle 22 and Their Solar Sources

Details Geomagnetic Disturbances Around the Solar Minimum of Cycle 22 and Their Solar Sources Geomagnetic Disturbances Around the Solar Minimum of Cycle 22 and Their Solar Sources

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..199w&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

Scientific paper

The solar sources of geomagnetic disturbances around the solar minimum of cycle 22 were investigated using in situ solar wind observations and solar observations from space. About half of the geomagnetic disturbances were associated with coronal mass ejections (CMEs). Approximately 20% of the geomagnetic disturbances were associated with both CMEs and high-speed solar wind streams. It was found that geomagnetic disturbances associated with CMEs tend to have large magnitudes and those associated with high-speed solar wind streams tend to have long durations.

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