Solar cycle variation of long duration 10.7 CM and soft X-ray bursts

Details Solar cycle variation of long duration 10.7 CM and soft X-ray bursts Solar cycle variation of long duration 10.7 CM and soft X-ray bursts

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115..385k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 115, no. 2, 1988, p. 385-396.

Physics

9

Long Term Effects, Solar Cycles, Solar X-Rays, Stellar Mass Ejection, Annual Variations, Bursts, Interplanetary Medium, Solar Corona, Solar Flux Density

Scientific paper

The authors use reports from the Ottawa and Penticton stations to examine the annual variations from 1965 to 1985 of 10.7 cm gradual rise-and-fall bursts with total durations of at least 4 hr. Four-hour events are more easily detected in X-ray data than in 10.7 cm data at solar minimum, but, conversely, these events are much more easily detected in 10.7 cm data around solar maximum. About 70% of the most energetic coronal mass ejection (CMEs) are associated with ≥4 hr X-ray or 10.7 cm bursts.

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