The solar chromospheric supergranular network in 850 micron radiation

Details The solar chromospheric supergranular network in 850 micron radiation The solar chromospheric supergranular network in 850 micron radiation

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...383..443l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 383, Dec. 10, 1991, p. 443-449.

Astronomy and Astrophysics

Astrophysics

11

Chromosphere, Infrared Spectra, Solar Atmosphere, Solar Granulation, Solar Spectra, K Lines, Solar Activity, Solar Magnetic Field, Solar Radio Emission

Scientific paper

The first submillimeter solar observations are examined of the chromospheric supergranular network, made on the 15-m James Clerk Maxwell Telescope on Mauna Kea in 850-micron radiation. These observations are useful for thermal diagnostics of the low and middle chromospheres of the quiet-sun and magnetic regions, where mechanical heating of the atmospheric medium first becomes manifest. The models of Vernazza, Avrett and Loeser appear to be consistent with these observations.

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