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A Brief History of Radio Astronomy in the USSRRadio Astronomy Studies at the Lebedev Physical Institute

A Brief History of Radio Astronomy in the USSR: Radio Astronomy Studies at the Lebedev Physical... [The history of the development of radio astronomy studies at FIAN is described, beginning with the first theoretical (1946) and experimental (1947) studies of the solar radio emission. Information about the development of the Crimean station of FIAN, then the establishment and development of the Radio Astronomy Station in Pushchino is presented. Work on the construction of large radio telescopes, including the FIAN 22-m, DKR-1000 and BSA telescopes, is described, together with important results obtained during observations of the Sun (including the discovery of its “supercorona”), planets, line radio emission and studies of pulsars and other discrete sources.] http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png

A Brief History of Radio Astronomy in the USSRRadio Astronomy Studies at the Lebedev Physical Institute

Part of the Astrophysics and Space Science Library Book Series (volume 382)
Editors: Braude, S. Y.; Salomonovich, A. E.; Samanian, V. A.; Shklovskii, I. S.; Sorochenko, R. L.; Troitskii, V. S.; Kellermann, K. I.; Dubinskii, B. A.; Kaidanovskii, N. L.; Kardashev, N. S.; Kobrin, M. M.; Kuzmin, A. D.; Molchanov, A. P.; Pariiskii, Yu. N.; Rzhiga, O. N.

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Publisher
Springer Netherlands
Copyright
© Springer Science+Business Media B.V. 2012
ISBN
978-94-007-2833-2
Pages
1 –60
DOI
10.1007/978-94-007-2834-9_1
Publisher site
See Chapter on Publisher Site

Abstract

[The history of the development of radio astronomy studies at FIAN is described, beginning with the first theoretical (1946) and experimental (1947) studies of the solar radio emission. Information about the development of the Crimean station of FIAN, then the establishment and development of the Radio Astronomy Station in Pushchino is presented. Work on the construction of large radio telescopes, including the FIAN 22-m, DKR-1000 and BSA telescopes, is described, together with important results obtained during observations of the Sun (including the discovery of its “supercorona”), planets, line radio emission and studies of pulsars and other discrete sources.]

Published: Nov 15, 2011

Keywords: Brightness Temperature; Radio Emission; Radio Telescope; Radio Astronomy; Crimean Station

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