Abstract The distance distribution of Coronal Mass Ejections (CMEs) with respect to the Heliomagnetic Current Sheet is studied. The analysis is carried out for all CMEs observed by the Solar Maximum Mission Satellite, years 1980 and 1984–86. We foud that during solar minimum times the CMEs are better associated with the heliomagnetic equator than at solar maximum.
The association of Coronal Mass Ejections during solar maximum times with the heliomagnetic current sheet
Advances in Space Research ; 13 , 9 ; 183-186
1993-01-01
4 pages
Article (Journal)
Electronic Resource
English
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