The Fe XIV and Fe X Corona at Solar Minimum

Details The Fe XIV and Fe X Corona at Solar Minimum The Fe XIV and Fe X Corona at Solar Minimum

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.2506a&link_type=abstract

American Astronomical Society Meeting 210, #25.06; Bulletin of the American Astronomical Society, Vol. 39, p.132

Astronomy and Astrophysics

Astronomy

Scientific paper

Although the solar disk is often devoid of sunspots around solar minimum, the upper atmosphere never rests. The most prominent features at the absolute minimum of coronal activity are dense regions overlying high latitude boundaries of the large scale magnetic field. Seen above the limb, these features typically give the impression of "ears" (and "jowls"). Samples of these features will be shown and their cause (the "extended solar cycle" running from near the poles to the equator over 18 years) explained. The author was supported by the Air Force Office of Scientific Research.

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