Handbook on Radio Astronomy
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Handbook on Radio Astronomy

The Handbook on Radio Astronomy has been developed by experts of Working Party 7D of ITU-R Study Group 7 (Science Services) that is responsible for radio astronomy. This Handbook is not intended as a source book on radio astronomy, but rather deals with such aspects of radio astronomy that are relevant to frequency coordination as the management of radio spectrum usage in order to minimize interference between radiocommunication services.

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Vulnerability of radio astronomy observations to interference You do not have access to this content

English
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Author(s):
ITU

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The radiation measured in radio astronomy has, in almost all cases, a Gaussian probability distribution in amplitude. Except in the case of narrow-band spectral line emissions, it has the same statistical characteristics as thermal noise radiation from the Earth, its atmosphere, or noise generated in a receiver itself. Moreover, the cosmic radio emissions are very weak. In radio astronomy observations, the S/N in the RF and IF parts of the receiver is typically in the range -20 dB to –60 dB, i.e. the power contributed by the source under study is a factor of 10–2 to 10–6 lower than the unwanted noise power from the atmosphere, the ground, and the receiver circuits. In most communication systems the corresponding S/N is of the order of unity or greater. Because radio astronomy signals are so weak in comparison to those of other services, radio astronomy observations are highly vulnerable to radio interference and, except in the case of pulsars, cosmic signals generally have no characteristic modulation that would help to distinguish them from noise or from many forms of interfering signals.