Solar Spectroscopy and Diagnostics: X-ray Emission

Details Solar Spectroscopy and Diagnostics: X-ray Emission Solar Spectroscopy and Diagnostics: X-ray Emission

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2234g&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2234. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Solar Observation

Scientific paper

X-ray emission from the Sun arises primarily from the solar outer atmosphere, particularly the hot corona. During transient events, such as flares and coronal mass ejections, there is also enhanced emission of both soft and hard x-rays from plasma above ten million kelvins (see SOLAR FLARES: RELATION TO CORONAL MASS EJECTIONS). Outside of flares, the bulk of the coronal plasma is at temperatures ...

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