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The solar causes of geomagnetic storms with a gradual commencement

✍ Scribed by Bohumila Bednářová-Nováková

Book ID
112787446
Publisher
Springer
Year
1967
Tongue
English
Weight
180 KB
Volume
11
Category
Article
ISSN
0039-3169

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The dominant interplanetary phenomena causing intense magnetic storms are the interplanetary manifestations of fast coronal mass ejections (CMEs). Two interplanetary structures are important for the development of such class of storms, involving an intense and long duration Bs component of the IMF: