DocumentCode :
1940018
Title :
The 64 m Sardinia radio telescope optics design
Author :
Cortés-Medellín, Germán
Author_Institution :
Vertex RSI, Santa Clara, CA, USA
Volume :
4
fYear :
2002
fDate :
2002
Firstpage :
136
Abstract :
The Sardinia radio telescope (SRT) is a project proposed by the Institute of Radio Astronomy (IRA, in Bologna, Italy). The SRT with a diameter of 64 m will be the third and largest Italian radio telescope. Designed to accommodate several instruments with a frequency coverage from 0.30 GHz to 100 GHz. In addition to the radio astronomy science applications, this instrument will be used for deep space communication missions in conjunction with the Italian Space Agency, as well as for geodynamic studies. The configuration of the Sardinia radio telescope is a symmetrical shaped Gregorian system with an aperture diameter of 64 m, and a 7.9 m diameter subreflector.
Keywords :
optics; radioastronomical techniques; radiotelescopes; reflector antennas; space communication links; 0.30 to 100 GHz; 3.95 m; 32 m; Bologna; Institute of Radio Astronomy; Italian Space Agency; Italy; Sardinia radio telescope; aperture diameter; deep space communication missions; frequency coverage; geodynamic studies; optics design; radio astronomy science applications; subreflector; symmetrical shaped Gregorian system; Focusing; Frequency; Instruments; Optical control; Optical design; Optical interferometry; Optical receivers; Radio astronomy; Reflector antennas; Space missions;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Antennas and Propagation Society International Symposium, 2002. IEEE
Print_ISBN :
0-7803-7330-8
Type :
conf
DOI :
10.1109/APS.2002.1016944
Filename :
1016944
Link To Document :
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