The Properties of the Solar Corona and Its Connection to the Solar Wind

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Ion Cyclotron Damping in the Solar Corona and Solar Wind

The solar corona is the hot, ionized outer atmosphere of the Sun. Coronal plasma expands into interplanetary space as a supersonic bulk outflow known as the solar wind. This tenuous and unbounded medium is a unique laboratory for the study of kinetic theory in a nearly collisionless plasma, as well as magnetohydrodynamic waves, shocks, and jets. Particle velocity distributions in the solar wind...

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ژورنال

عنوان ژورنال: Annual Review of Astronomy and Astrophysics

سال: 2019

ISSN: 0066-4146,1545-4282

DOI: 10.1146/annurev-astro-091918-104416