DocumentCode :
343531
Title :
Design features of the Large Millimeter Telescope (LMT)
Author :
Baars, J.W.M. ; Karcher, H.J.
Author_Institution :
Massachusetts Univ., Amherst, MA, USA
Volume :
3
fYear :
1999
fDate :
11-16 July 1999
Firstpage :
1544
Abstract :
Because astronomical millimeter observations are strongly impeded by atmospheric water vapor in the line of sight, MM-wave telescopes must be placed at high mountain sites with a dry atmosphere. The LMT will be located on Cerro la Negra in central Mexico at an altitude of 4600 m. The antenna is currently in the critical design phase at MAN Technologie, Germany. In this paper we summarize the salient features of the LMT design with particular reference to the special methods required to realize the stringent specifications for operation at 1 mm wavelength.
Keywords :
millimetre wave antennas; radiotelescopes; receiving antennas; reflector antennas; 1 mm; 50 m; Cerro la Negra; LMT; Large Millimeter Telescope; MM-wave telescopes; antenna; astronomical millimeter observations; central Mexico; design features; specifications; Detectors; Jacobian matrices; Millimeter wave technology; Optical design; Radio astronomy; Reflector antennas; Space technology; Submillimeter wave technology; Telescopes; Temperature measurement;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Antennas and Propagation Society International Symposium, 1999. IEEE
Conference_Location :
Orlando, FL, USA
Print_ISBN :
0-7803-5639-x
Type :
conf
DOI :
10.1109/APS.1999.788237
Filename :
788237
Link To Document :
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