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TVT, 1971, Volume 9, Issue 3, Pages 497–504 (Mi tvt10393)  

Plasma Investigations

Experimental investigation of the spectral characteristics of the Venusian atmosphere at high temperatures

A. A. Kon'kov, S. G. Kulagin

Institute for High Temperatures, USSR Academy of Sciences, Moscow

Abstract: The spectral composition of the radiation, the the emissivity and absorptivity of a mixture of $91%  CO_2$ and $9% \rm N_2$ are investigated, as having similar characteristics to the Martian and Venusian atmospheres. The experimental data are compared to theoretical calculations.

Full text: PDF file (448 kB)

English version:
High Temperature, 1971, 9:3, 453–459
UDC: 535.33
Received: 10.02.1970

Citation: A. A. Kon'kov, S. G. Kulagin, “Experimental investigation of the spectral characteristics of the Venusian atmosphere at high temperatures”, TVT, 9:3 (1971), 497–504; High Temperature, 9:3 (1971), 453–459

Citation in format AMSBIB
\Bibitem{KonKul71}
\by A.~A.~Kon'kov, S.~G.~Kulagin
\paper Experimental investigation of the spectral characteristics of the Venusian atmosphere at high temperatures
\jour TVT
\yr 1971
\vol 9
\issue 3
\pages 497--504
\mathnet{http://mi.mathnet.ru/tvt10393}
\transl
\jour High Temperature
\yr 1971
\vol 9
\issue 3
\pages 453--459
\scopus{http://www.scopus.com/record/display.url?origin=inward&eid=2-s2.0-0015066617}


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