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...

Deskribapen osoa

Xehetasun bibliografikoak

Egile Nagusiak:	Laurel A. Rachmeler, Sarah E. Gibson, Stephen M. White
Formatua:	Online
Hizkuntza:	ingelesa
Argitaratua:	Frontiers Media SA 2021
Gaiak:	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
Sarrera elektronikoa:	24024
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