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Determination of the spread function for solar stray light

โœ Scribed by L. Staveland

Book ID
104672508
Publisher
Springer
Year
1970
Tongue
English
Weight
176 KB
Volume
12
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

On the instrumental and atmospheric stra
On the instrumental and atmospheric stray-light for solar observations
โœ W. Mattig ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 331 KB

From aureole measurements made with a 40 cm-Vacuum-Telescope at Izafia (Tenerife) in the wavelength region 417 nm < 2 < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin. (b)

A Gaussian spread function for the solar
A Gaussian spread function for the solar aureole
โœ L. Staveland ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 124 KB

An analytical expression for the limb profile and the aureole is derived for a Gaussian spread function with b/> 2'. Power series with 3 terms are used as approximation to the limb darkening given by HSRA (Gingerich et al., 1971). For smaller values of the spread parameter b the expression given by