Irregularities of the limb of the solar disk in white light

Details Irregularities of the limb of the solar disk in white light Irregularities of the limb of the solar disk in white light

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59..186d&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, Jan.-Feb. 1982, p. 186-189.) Soviet Astronomy, vol. 26, Jan.-Feb. 1982, p. 113, 114. Transl

Astronomy and Astrophysics

Astronomy

Continuous Spectra, H Alpha Line, Solar Granulation, Solar Limb, Solar Spectra, Atmospheric Turbulence, Light (Visible Radiation), Solar Atmosphere, Statistical Analysis

Scientific paper

At the very limb of the solar disk the continuous spectrum is broken up
into separate strips, which we consider as a manifestation of the
irregularity ('hilliness') of the limb of the solar disk. The distance
between the strips correspond to the sizes of supergranules. The height
of the 'hills' is on the order of 400 km.

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