Magnetic measurements of coronal holes during 1975-1980

Details Magnetic measurements of coronal holes during 1975-1980 Magnetic measurements of coronal holes during 1975-1980

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79..149h&link_type=abstract

Solar Physics, vol. 79, July 1982, p. 149-160.

Physics

40

Coronal Holes, Magnetic Flux, Magnetic Measurement, Photosphere, Solar Magnetic Field, Interplanetary Magnetic Fields, Solar Atmosphere, Sunspot Cycle

Scientific paper

Low latitude coronal holes are found to contain three times more flux near sunspot maximum than near minimum, despite the similarity of sizes in the two conditions, by measurements of photospheric magnetic fluxes and average field strengths beneath 33 coronal holes observed on 63 occasions during 1975-1980. Average magnetic field strengths ranged from 3-36 G near sunspot maximum, and 1-7 G near minimum. It is suggested that the low latitude coronal holes received a proportion of the extra flux available at low latitudes near sunspot maximum. The coronal hole magnetic measurements are presented in tabular form.

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