A dynamic thermal model for design and control of an 800-element open-air radio telescope
2011
In earlier work we have described the thermal modelling for design and
control of a fully insulated, and sometimes ventilated, high precision
radio telescope. For such an insulated telescope the modelling of the
time-variable dynamic influence of the thermal environment (air, sky
and ground radiation, insolation) is relatively simple. The modelling
becomes however quite complex for an open-air radio telescope where
each individual member of the reflector backup structure (BUS) and the
support structure (fork or yoke) is exposed under a different and
time-dependent aspect angle to the thermal environment, which applies
in particular to solar radiation. We present a time-dependent
800-element thermal model of an open-air telescope. Using the IRAM
30-m radio telescope as the basic mechanical structure, we explain how
the temperature induced, real-time pointing and reflector surface
deformations can be derived when using as input the day of the year,
the thermal environment, and the geographic position of the telescope
and its changing pointing direction. Thermal modelling and results
similar to those reported here can be used for radio telescope design
and real-time control of pointing and surface adjustment of a
telescope with active panels.
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