DocumentCode :
2722846
Title :
The LOFAR phased array telescope system
Author :
Gunst, André W. ; Bentum, Mark J.
Author_Institution :
ASTRON, Dwingeloo, Netherlands
fYear :
2010
fDate :
12-15 Oct. 2010
Firstpage :
632
Lastpage :
639
Abstract :
The Low Frequency Array (LOFAR) is the largest telescope in the world operating at a frequency range from 30 to 240 MHz. LOFAR is the first radio telescope of its size which uses phased array principles to detect radio signals. More than 10,000 antennas are installed in the field. The antennas are grouped in 44 stations. The maximal distance between the stations is about 1500 km resulting in a tremendous spatial resolution. In this paper the LOFAR system architecture is discussed and the status is described.
Keywords :
antenna phased arrays; radioastronomy; radiotelescopes; LOFAR phased array telescope system; Low Frequency Array; frequency 30 MHz to 240 MHz; phased array principles; radio signal detection; radiotelescope; Antennas; Arrays; Correlation; Correlators; Filter bank; Instruments; Sensors;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Phased Array Systems and Technology (ARRAY), 2010 IEEE International Symposium on
Conference_Location :
Waltham, MA
Print_ISBN :
978-1-4244-5127-2
Electronic_ISBN :
978-1-4244-5128-9
Type :
conf
DOI :
10.1109/ARRAY.2010.5613300
Filename :
5613300
Link To Document :
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