HELIOSPHERIC PROPAGATION OF CORONAL MASS EJECTIONS: DRAG-BASED MODEL FITTING
نویسندگان
چکیده
منابع مشابه
Role of coronal mass ejections in the heliospheric Hale cycle
[1] The 11-year solar cycle variation in the heliospheric magnetic field strength can be explained by the temporary buildup of closed flux released by coronal mass ejections (CMEs). If this explanation is correct, and the total open magnetic flux is conserved, then the interplanetary-CME closed flux must eventually open via reconnection with open flux close to the Sun. In this case each CME wil...
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ژورنال
عنوان ژورنال: The Astrophysical Journal Supplement Series
سال: 2015
ISSN: 1538-4365
DOI: 10.1088/0067-0049/218/2/32