Solar Corona: X-ray Bright Points

Details Solar Corona: X-ray Bright Points Solar Corona: X-ray Bright Points

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2022p&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2022. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Solar Atmosphere

Scientific paper

X-ray (or coronal) bright points are small knots of intense x-ray
emission scattered randomly throughout the solar CORONA. They are
associated with pairs of opposite-polarity magnetic flux seen below in
the SOLAR PHOTOSPHERE and are most likely to be heated by the motion of
the magnetic fluxes causing reconnection in the corona....

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