Published October 1983 | Version v1
Journal article

On the integration of intensity measurements of the solar center and limb near 300 nanometers

Creators

Description

Two methods of integrating limb-darkening data to calculate the spectral irradiance are compared. Near 30 nm Moe and Milone's (1978) quadratic approximation to the limb darkening yields an integral 3% larger on average than the two linear segments of Kohl et al. (1980) when the same data are inserted in both formulas. As one would expect, the difference between the two calculations is directly proportional to Moe and Milone's quadratic coefficient. When Moe and Milone's data are inserted in the formula of Kohl et al., the calculated irradiance is 4% higher than when the data of Kohl et al. are used in the same formula. Possible reasons for this difference are suggested. (orig.)

Additional details

Publishing Information

Journal Title
Sol. Phys.
Journal Volume
88
Journal Issue
1/2
Series
CODEN: SLPHA.;Sol. Phys.
Journal Page Range
9-12
ISSN
0038-0938

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
15011523
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
RADIATION FLUX; SOLAR RADIATION; SPATIAL DISTRIBUTION; SUN; VISIBLE RADIATION
Descriptors DEC
DISTRIBUTION; ELECTROMAGNETIC RADIATION; MAIN SEQUENCE STARS; RADIATIONS; STARS; STELLAR RADIATION