Sensitivity of Antenna Arrays for Long-Wavelength Radio Astronomy

A number of new and planned radio telescopes will consist of large arrays of low-gain antennas operating at frequencies below 300 MHz. In this frequency regime, Galactic noise can be a significant or dominant contribution to the total noise. This, combined with mutual coupling between antennas, make...

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Bibliographic Details
Published inIEEE transactions on antennas and propagation Vol. 59; no. 6; pp. 1855 - 1863
Main Author Ellingson, S W
Format Journal Article
LanguageEnglish
Published New York IEEE 01.06.2011
The Institute of Electrical and Electronics Engineers, Inc. (IEEE)
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