Course : Εισαγωγή στη Ραδιοστρονομία
Course code : PH338C
Definition
The study of astronomical objects through electromagnetic radiation at radio wavelengths, roughly from millimetres to tens of metres.
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Definition
An equation that estimates the sensitivity of a radio observation based on system temperature, bandwidth, integration time, and number of polarizations.
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Definition
The electronic system that amplifies and processes the weak signal collected by the antenna.
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Definition
Noise added by the telescope electronics.
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Definition
A quantity describing the amount of Faraday rotation. It depends on the electron density, magnetic field, and path length through the plasma.
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