Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 120, Number 1, November_II 1996
Page(s) 35 - 39
DOI https://doi.org/10.1051/aas:1996272
Published online 15 November 1996
On the consistency of solar limb darkening observations at UV wavelengths (2000 -3300 Å) DOI: 10.1051/aas:1996272

Astronomy and Astrophysics Supplement Series, Vol. 120, November II 1996, 35-39

On the consistency of solar limb darkening observations at UV wavelengths (2000 -3300 Å)

A. Greve and H. Neckel
Send offprint requests to: A. Greve

Institut de Radioastronomie Millimetrique, 300 Rue de la Piscine, 38406 St. Martin d`Hères, France
Hamburger Sternwarte, 112 Gojenbergweg, 21029 Hamburg, Germany

Received February 12; accepted April 5, 1996

Abstract:

Limb darkening observations are important for the construction and verification of solar model atmospheres. We investigate the consistency of solar limb darkening data, published for the UV wavelength region between 2000 and 3300 Å, from the comparison of ratios based either on direct limb darkening observations or on absolute irradiance (F) and disk--center intensity () measurements. There exists a discrepancy between the limb darkening data of Moe & Milone and other, direct or indirect, limb darkening observations.

Key words: Sun: atmosphere --- UV radiation


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