Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006asthe..99..675k&link_type=abstract
The Astronomical Herald (ISSN 0374-2466), Vol. 99, No. 12, p. 675 - 681 (2006)
Astronomy and Astrophysics
Astronomy
Geomagnetic Field, Radiation Belts, Solar Wind
Scientific paper
Radiation belts show various patterns of evolution during a few days after a magnetic storm onset, and the prediction has been a difficult problem. Using a 10 year data set of the sun, solar wind, radiation belts, and geomagnetic field, we show that the outer radiation belt tends to be more dangerous for geosynchronous satellites than usual during storms associated with coronal holes, and that the outer radiation belt tends to be rather safe during storms associated with coronal mass ejections. In this paper, we report our new findings and introduce a practical aspect of space weather forecast of radiation belts for secure satellite operations.
Kataoka Ryuho
Miyoshi Yoshizumi
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