Estimates of convective heat fluxes and gravity wave amplitudes in the Venus middle cloud layer from VEGA balloon measurements-Reference-Cited by-同舟云学术

Estimates of convective heat fluxes and gravity wave amplitudes in the Venus middle cloud layer from VEGA balloon measurements

Published:1987-01 Issue:12 Volume:7 Page:343-349
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Ingersoll A.P.,Crisp D.,Grossman A.W.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference8 articles.

1. Greenhouse models of Venus' high surface temperature, as constrained by Pioneer Venus measurements;Pollack;J. Geophys. Res.,1980

2. Overview of VEGA Venus balloon in-situ meteorological measurements;Sagdeev;Science,1986

3. Thermal structure of the Venus atmosphere in the middle cloud layer;Linkin;Science,1986

4. L.S. Elson and the VEGA Balloon Science Team, Meteorological variations in the middle clouds of Venus from VEGA balloon in-situ measurements, this issue

5. VEGA balloon dynamics and vertical winds in the Venus middle cloud region;Linkin;Science,1986

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