Digital image processing of the CCD (SRT) positional observations of two satellites (Ariel and Titania) of Uranus.

Details Digital image processing of the CCD (SRT) positional observations of two satellites (Ariel and Titania) of Uranus. Digital image processing of the CCD (SRT) positional observations of two satellites (Ariel and Titania) of Uranus.

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acasn..39..320p&link_type=abstract

Acta Astron. Sin., Vol. 39, No. 3, p. 320 - 323

Astronomy and Astrophysics

Astronomy

Image Processing: Uranus Satellites, Positions: Uranus Satellites

Scientific paper

The positional determination of natural satellites is very important in astrometry and celestial mechanics. Some researchers have performed very good astrometric observations of Uranian satellites with a new image processing technique. The authors compared the methods without and with halo-processing for the CCD (SRT-Separated Readout Technique) observations of Ariel and Titania carried out with the 1-meter telescope of Yunnan Observatory. When the two satellites were used to determine the CCD scale and orientation, it was clarified that the Uranian halo-processing is very important for the positional determination of satellites.

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