Estimating the possible ammonia content in the atmosphere of Venus-Reference-Cited by-同舟云学术

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Estimating the possible ammonia content in the atmosphere of Venus

Published:1976-01 Issue:1 Volume:19 Page:1-6
ISSN:0033-8443
Container-title:Radiophysics and Quantum Electronics
language:en
Short-container-title:Radiophys Quantum Electron

Author:

Naumov A. P.,Zinicheva M. B.,Muratov N. N.

Publisher

Springer Science and Business Media LLC

Subject

Electrical and Electronic Engineering,Astronomy and Astrophysics,Nuclear and High Energy Physics,Statistical and Nonlinear Physics,Electronic, Optical and Magnetic Materials

Link

http://link.springer.com/content/pdf/10.1007/BF01038400.pdf

Reference64 articles.

1. V. I. Moroz, Physics of the Planets [in Russian], Izd. Nauka, Moscow (1967).

2. A. D. Kuz'min, Radiophysics Investigations of Venus [in Russian], VINITI AN SSSR, Moscow (1967).

3. Yu. M. Timofeev, M. A. Gruzdeva, and O. M. Pokrovskii, Radiation Transfer in the Atmosphere [in Russian], Izd. LGU (1972), p. 108.

4. Yu. A. Surkov, B. M. Andreichikov, and O. M. Kalinkina, Dokl. Akad. Nauk SSSR,213, No. 2, 296 (1971).

5. T. V. Smirnova and A. D. Kuz'min, Astron. Zh.,51, No. 3, 607 (1974).

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