Coronal holes and photospheric magnetic fields

Details Coronal holes and photospheric magnetic fields Coronal holes and photospheric magnetic fields

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..890o&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, July-Aug. 1990, p. 890-893. In Russian.

Computer Science

Sound

8

Coronal Holes, Photosphere, Solar Cycles, Solar Magnetic Field, Energy Dissipation, Solar Flux Density, Solar Radiation, Sound Waves

Scientific paper

Magnetic field observations reported by Hoeksema and Scherrer (1986) were used to examine the mutual arrangement of coronal holes recorded in the 10830 He I line during the fall-off phase (1982-1985) of the 21st solar cycle, relative to the large-scale photospheric and coronal magnetic fields. Results show that the coronal holes change in phase with the total solar radiation flux in the Ca II line, indicating their common nature. A mechanism for heating coronal holes, similar to that proposed by Pikel'ner (1960), is discussed.

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