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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Egile nagusia: Laurel A. Rachmeler (auth)
Beste egile batzuk: Sarah E. Gibson (auth), Stephen M. White (auth)
Formatua: Liburu kapitulua
Argitaratua: Frontiers Media SA 2017
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