Desgin and software aspects for the control system of the 30 m MRT.

Details Desgin and software aspects for the control system of the 30 m MRT. Desgin and software aspects for the control system of the 30 m MRT.

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984spie..444q.122s&link_type=abstract

Proc. SPIE Int. Soc. Opt. Eng., Vol. 444, p. 122 - 126

Computer Science

Performance

Radio Telescopes:Sub-Mm Radiation, Sub-Mm Radiation:Radio Telescopes

Scientific paper

The 30 m Millimeter Radiotelescope (MRT) will have a beamwidth of less than 10arcsec when operated at a wavelength of 1.2 mm. It is an open air telescope located on a mountain ridge in southern Spain. There the instrument is exposed to severe environmental influences, especially wind and temperature changes. The pointing and tracking accuracy required is of the order of a few seconds of arc. Simulations have shown that these specifications cannot be met with conventional servo design. An improvement of performance can be obtained applying the modern concept of state control.

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