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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Detalles Bibliográficos

Main Authors:	Laurel A. Rachmeler, Sarah E. Gibson, Stephen M. White
Formato:	Online
Idioma:	inglés
Publicado:	Frontiers Media SA 2021
Subjects:	QB1-991 Q1-390 solar corona Solar Activity magnetohydrodynamics solar flares Coronal mass ejections Magnetic Fields spectropolarimetry Sun thema EDItEUR::P Mathematics and Science::PG Astronomy, space and time
Acceso en liña:	24024
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