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Coronal Magnetometry

Magnetism defines the complex and dynamic solar corona. It determines the magnetic loop structure that dominates images of the corona, and stores the energy necessary to drive coronal eruptive phenomena and flare explosions. At great heights the corona transitions into the ever-outflowing solar wind...

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Bibliographic Details
Main Author: Laurel A. Rachmeler (auth)
Other Authors: Sarah E. Gibson (auth), Stephen M. White (auth)
Format: Electronic Book Chapter
Language:English
Published: Frontiers Media SA 2017
Series:Frontiers Research Topics
Subjects:
Astronomy, space & time
solar corona
Solar Activity
magnetohydrodynamics
solar flares
Coronal mass ejections
Magnetic Fields
spectropolarimetry
Sun
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