The development of structure in the quiet solar chromosphere

Details The development of structure in the quiet solar chromosphere The development of structure in the quiet solar chromosphere

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..138k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Mar. 1979, p. 138-142.) Soviet Astronomy Letters, vol. 5, Mar.-Apr. 1979, p. 75-77.

Astronomy and Astrophysics

Astronomy

Chromosphere, Fine Structure, Solar Atmosphere, Stellar Structure, H Alpha Line, K Lines, Solar Spectra, Time Dependence

Scientific paper

A discussion is given of the energy balance in the region of the solar chromosphere that becomes compressed as a supergranule forms. Initially the compression will be accompanied by rapid heating, but subsequently the temperature excess will gradually be radiated away, whereas the density will continue to rise until new supergranules develop and destroy the cooled elements of the network. The influence of this process on the chromospheric structure observable in the H-alpha and Ca II K lines is examined.

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