Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spie.3737...32a&link_type=abstract
Proc. SPIE Vol. 3737, p. 32-36, Design and Engineering of Optical Systems II, Fritz Merkle; Ed.
Astronomy and Astrophysics
Astronomy
2
Scientific paper
Converting linear coordinates in the plane of the detector of an astronomical instrument to celestial coordinates involves in principle the equivalent focal length of the instrument. However, most methods in astrometry manage to reduce observations in a global manner without actually measuring a focal length. We point out a case for solar space observations where the long term stability of angular distance measurements is better than the ground calibration of the angular value of a pixel. We report and discuss this ground calibration.
Artzner Guy E.
Auchere Frédéric
Delaboudinière Jean Pierre
Hochedez Jean-Francois E.
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