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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Published in | IEEE transactions on antennas and propagation Vol. 59; no. 6; pp. 1855 - 1863 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
New York
IEEE
01.06.2011
The Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
Subjects | |
Online Access | Get full text |
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