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

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

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..120...35g&link_type=abstract

Astronomy and Astrophysics Supplement, v.120, p.35-39

Astronomy and Astrophysics

Astrophysics

7

Sun: Atmosphere, Uv Radiation

Scientific paper

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 3300A, from the comparison of F/I_0_ ratios based either on direct limb darkening observations or on absolute irradiance (F) and disk-center intensity (I_0_) measurements. There exists a discrepancy between the limb darkening data of Moe & Milone (1978ApJ...226..301M) and other, direct or indirect, limb darkening observations.

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