Associations between coronal mass ejections and soft X-ray events

Details Associations between coronal mass ejections and soft X-ray events Associations between coronal mass ejections and soft X-ray events

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...272..349s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 272, Sept. 1, 1983, p. 349-354.

Astronomy and Astrophysics

Astrophysics

154

Solar Corona, Solar X-Rays, Stellar Mass Ejection, Statistical Analysis, Sunspots

Scientific paper

The association between white light coronal mass ejections (CMEs) and full-disk X ray events have been examined as a function of X ray duration during the recent years of high sunspot activity (1979-1981). On a time scale of hours, no duration interval has been found that separates X ray events into two distinct classes depending on whether or not they have associated CMEs. Rather, the tendency for long-duration X ray events to have associated CMEs reflects the fact that, as X ray duration increases, the differential distribution of events without CMEs falls off faster than the distriution of X ray events with CMEs.

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