𝔖 Bobbio Scriptorium
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Solar storms, Mars and a comet’s tail

✍ Scribed by Peter Bond

Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
889 KB
Volume
41
Category
Article
ISSN
1366-8781

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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: