Title :
An overview of the Green Bank Telescope
Author :
Srikanth, S. ; Norrod, R. ; King, L. ; Parker, D.
Author_Institution :
Nat. Radio Astron. Obs., Charlottesville, VA, USA
Abstract :
The Green Bank Telescope (GBT) at the National Radio Astronomy Observatory (NRAO) site in Green Bank, is to be the largest, fully-steerable telescope in the world. The GBT has a main reflector 100 m/spl times/100 m with unblocked aperture. The telescope will operate at prime focus in the 230 MHz-1200 MHz frequency range and at Gregorian focus in the 1.15 GHz to >100 GHz range. The performance of the GBT above 15 GHz will be enhanced by the use of an active surface and a metrology system. The location of the surface panels are to be measured and adjusted to minimize the surface error as measured from a best-fit paraboloid. Switching between prime focus and secondary focus operation, as well as selection of different receivers, will be achieved in a few minutes giving the telescope a rapid frequency agility.
Keywords :
UHF antennas; antenna accessories; antenna radiation patterns; microwave antennas; millimetre wave antennas; offset reflector antennas; radiotelescopes; receiving antennas; 100 m; 110 m; 290 MHz to 100 GHz; Green Bank Telescope; Gregorian focus; National Radio Astronomy Observatory site; active surface; frequency agility; fully-steerable telescope; main reflector; metrology system; prime focus; secondary focus; surface error; surface panels; Apertures; Azimuth; Extraterrestrial measurements; Feeds; Frequency; Metrology; Observatories; Optical surface waves; Radio astronomy; Telescopes;
Conference_Titel :
Antennas and Propagation Society International Symposium, 1999. IEEE
Conference_Location :
Orlando, FL, USA
Print_ISBN :
0-7803-5639-x
DOI :
10.1109/APS.1999.788238