Area variation with temperature of supergranule network features in the solar transition zone

Details Area variation with temperature of supergranule network features in the solar transition zone Area variation with temperature of supergranule network features in the solar transition zone

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...58...31e&link_type=abstract

Solar Physics, vol. 58, June 1978, p. 31-36. USAF-supported research

Physics

1

Far Ultraviolet Radiation, Solar Corona, Solar Granulation, Solar Temperature, Spectroheliographs, Abundance, Carbon, Chromosphere, Emission Spectra, Oxygen

Scientific paper

Areas of network emission features in C II 1135 A, C III 977 A, O IV 544 A, and O VI 1032 A were measured in and out of coronal holes. In the quiet sun these areas, on the average, showed a 20% increase between C II and O VI. In the coronal holes there was no significant average variation, but a number of the features showed an interesting decrease in area at intermediate temperatures.

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