Motion of the Large European Solar Telescope (LEST) mounting

Details Motion of the Large European Solar Telescope (LEST) mounting Motion of the Large European Solar Telescope (LEST) mounting

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982lest.rept..194b&link_type=abstract

In its LEST: Large European Solar Telescope p 194-198 (SEE N82-32209 22-89)

Physics

Reflecting Telescopes, Solar Instruments, Translational Motion, Declination, Mounting, Optical Tracking, Series Expansion, Zenith

Scientific paper

The motion of the large European solar telescope about two axes of rotation, defined by the zenith and a point (R) inclined at an angle of 90 deg minus the value of a given angle (i) is analyzed. The telescope is assumed to track the Sun at different times of the year, and to be located at 28 deg N. The telescope is connected to the upper hemisphere in K, at a position 90 deg minus q from R. If the telescope is required to point at the zenith, it is shown that q = 90 deg - i must be defined. Two solutions, defined by solar declination limits, are possible and can be selected depending on the time of day.

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