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Temperature fluctuations in the solar photosphere

โœ Scribed by P. R. Wilson


Publisher
Springer
Year
1969
Tongue
English
Weight
767 KB
Volume
9
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


Temperature fluctuations in the solar ph
โœ P. R. Wilson ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 890 KB

The general problem of interpreting granulation data, in particular Edmonds' r.m.s. intensity fluctuation distribution against heliocentric angle 0, is discussed. A inethod is developed for investigating a variety of models of inhomogelaeous departures fi'om radiative equilibrium using two dimensio

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From the variations in equivalent width of a selected set of Fraunhofer lines, we derived the variation of effective temperature and microturbulence velocity between the equator and the regions at heliographic latitude of ~ 72 ~ The reliability of the results (AT/T--O:kO.6 %, A~/ff --6 % ~ 13 %) nee

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Amplitude distributions, which are nearly Gaussian, have been calculated for radial velocity, continuum brightness, spectral line equivalent width and spectral line central residual intensity fluctuations measured from high-dispersion high-resolution spectrograms taken at the center of the solar dis

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Residual intensity fluctuation measurements within the wings of the 25183.6 MgI bl line, obtained from two, high-resolution, high-dispersion, Sacramento Peak Observatory spectrograms, have been subtracted from intensity fluctuations in the adjacent continuum in order to isolate fluctuations associat