Structure of a Large low-Latitude Coronal Hole

Details Structure of a Large low-Latitude Coronal Hole Structure of a Large low-Latitude Coronal Hole

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..193..181b&link_type=abstract

Solar Physics, v. 193, Issue 1/2, p. 181-193 (2000).

Physics

19

Scientific paper

Coronal holes on the Sun are the source of high-speed solar wind streams that produce magnetic disturbances at the Earth. A series of multi-wavelength, multi-instrument observations obtained during the 1996 `Whole Sun Month' campaign examined a large coronal hole in greater detail than ever before. It appeared on the Sun in August, and extended from the north pole to a large active region in the southern hemisphere. Its physical and magnetic structure and subsequent evolution are described.

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