Structure of the solar atmosphere as deduced from a reanalysis of limb darkening observations

Details Structure of the solar atmosphere as deduced from a reanalysis of limb darkening observations Structure of the solar atmosphere as deduced from a reanalysis of limb darkening observations

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...244..511j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 2, April 1991, p. 511-520.

Astronomy and Astrophysics

Astrophysics

4

Astronomical Photometry, Continuous Spectra, Limb Darkening, Solar Atmosphere, Solar Limb, Absorption Spectra, Astronomical Models, Hydrogen Ions, Local Thermodynamic Equilibrium, Radiative Transfer

Scientific paper

A reanalysis of solar limb darkening measures with accurate central disk
intensities yields improved values of 'observed' absorption
coefficients, mean intensities, fluxes, and second moments, in the outer
layers of the sun. 'Observed' absorption coefficients are shown to be in
excellent agreement with the latest negative hydrogen ion data.

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