Abstract
I ν = 2kT B∕λ 2 and \(S_\nu =\int (2kT_{\mathrm {B}}/\lambda ^2) \mathrm {d}\varOmega =(2kT_{\mathrm {B}}/\lambda ^2) \varDelta \varOmega \).
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Wilson, T.L., Hüttemeister, S. (2018). Solutions for Chapter 7: Practical Aspects of Filled Aperture Antennas. In: Tools of Radio Astronomy - Problems and Solutions. Astronomy and Astrophysics Library. Springer, Cham. https://doi.org/10.1007/978-3-319-90820-5_23
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DOI: https://doi.org/10.1007/978-3-319-90820-5_23
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