Activity of Small-Scale Internal Waves in the Northern Polar Atmosphere of Venus by Radio Occultation Measurements of Signal Intensity (Λ = 32 cm) from Venera-15 and -16 Satellites-Reference-Cited by-同舟云学术

Activity of Small-Scale Internal Waves in the Northern Polar Atmosphere of Venus by Radio Occultation Measurements of Signal Intensity (Λ = 32 cm) from Venera-15 and -16 Satellites

Published:2021-01 Issue:1 Volume:55 Page:1-10
ISSN:0038-0946
Container-title:Solar System Research
language:en
Short-container-title:Sol Syst Res

Author:

Gubenko V. N.,Kirillovich I. A.,Gubenko D. V.,Andreev V. E.,Gubenko T. V.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1134/S0038094621010044.pdf

Reference25 articles.

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2. Crisp, D., Radiative forcing of the Venus mesosphere. II. Thermal fluxes, cooling rates, and radiative equilibrium temperatures, Icarus, 1989, vol. 77, pp. 391–413.

3. Fels, S.B., A parameterization of scale-dependent radiative damping grace in the middle atmosphere, J. Atmos. Sci., 1982, vol. 39, pp. 1141–1152.

4. Gubenko, V.N. and Andreev, V.E., Radio wave fluctuations and layered structure of the upper region of Venusian clouds from radio occultation data, Cosmic Res., 2003, vol. 41, no. 2, pp. 135–140.

5. Gubenko, V.N. and Kirillovich, I.A., The study of zonal circulation of Venus’s atmosphere by data analysis of radio occultation measurements made by Venera-15 and -16 satellites, Cosmic Res., 2018a, vol. 56, no. 6, pp. 471–479. https://doi.org/10.1134/S0010952518060047

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