Seeing-independent definitions of the solar limb position

Details Seeing-independent definitions of the solar limb position Seeing-independent definitions of the solar limb position

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...116..260b&link_type=abstract

Astronomy and Astrophysics, vol. 116, no. 2, Dec. 1982, p. 260-264.

Astronomy and Astrophysics

Astrophysics

6

Astrometry, Fourier Transformation, Solar Limb, Solar Position, Angular Distribution, Limb Darkening, Point Spread Functions

Scientific paper

The most important of the advantages of the finite Fourier transform definition (FFTD) is a low sensitivity to changes in the width of the atmospheric point spread function. This paper describes a class of similar edge definitions which share the advantages of the FFTD and which may be tailored to any desired limb darkening function or set of observing conditions. For some limb darkening functions, edge definitions may be obtained which are substantially less sensitive to seeing than the FFTD.

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