Solar limb darkening with allowance for absorption lines

Details Solar limb darkening with allowance for absorption lines Solar limb darkening with allowance for absorption lines

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...57o&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, Sept.-Oct. 1987, p. 57-64. In Russian.

Physics

Optics

2

Absorption Spectra, Electrophotometry, Limb Darkening, Line Spectra, Solar Limb, Atmospheric Optics, Light Scattering, Transparence

Scientific paper

The photoelectric scanning method is used to determine solar limb darkening in the integral (lines plus continuum) spectrum for 111 spectral regions (5-nm wide). The results obtained in Kiev (355-670 nm) are in agreement with those obtained on peak Terskol (317.5-362.5 nm). The following factors responsible for distortions are considered: atmospheric transparency fluctuations; and light scattering in the spectrograph, in the atmosphere, and on the telescope mirrors. Results are presented for nine positions on the solar disk.

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