Chemical Analysis of Materials Exposed to Venus Temperature and Surface Atmosphere [PDF]
Dorothy Lukco +8 more
openalex +1 more source
A fast equatorial jet in the Venusian cloud layer has been revealed by the Akatsuki orbiter by tracking cloud movement in near-infrared images. The findings suggest that the Venusian atmosphere is more variable than previously thought.
openaire +2 more sources
Venus general atmosphere circulation described by Pioneer [PDF]
The predominant weather pattern for Venus is described. Wind directions and wind velocities are given. Possible driving forces of the winds are presented and include solar heating, planetary rotation, and the greenhouse ...
core +1 more source
The upper atmosphere of Venus: Model predictions for mass spectrometry measurements
Salome Gruchola +3 more
openalex +2 more sources
Telecommunications and data acquisition support for the Pioneer Venus Project: Pioneers 12 and 13, prelaunch through March 1984 [PDF]
The support provided by the Telecommunications and Data Acquisition organization of the Jet Propulsion Laboratory (JPL) to the Pioneer Venus missions is described. The missions were the responsibility of the Ames Research Center (ARC).
Miller, R. B. +3 more
core +1 more source
The dynamics of a rapidly escaping atmosphere: Applications to the evolution of Earth and Venus
Andrew Watson +2 more
openalex +2 more sources
Mikhail Lomonosov and the discovery of the atmosphere of Venus during the 1761 transit [PDF]
M. Ya. Marov
openalex +1 more source
Airborne observations of astronomical objects [PDF]
The UV spectra of the sun, as well as the differences and ratios of planetary and solar spectra, are presented. The results indicate that SO, SO2 and ClO2 may be present in Venus' atmosphere, and Formaldehyde CH2O and ClO2 on Jupiter.
Sivjee, G. G.
core +1 more source
Absorption of sunlight in the atmosphere of Venus [PDF]
The profiles of upward, downward and net solar flux on Venus were measured at altitudes from about 62 km to the surface in three spectral bands at a vertical resolution of a few hundred meters.
Doose, L. R., Tomasko, M. G.
core +1 more source
Bounds on the thermodynamical properties of the fluid envelope of a planet based upon its radiative budget at the top of the atmosphere: theory and results for Earth, Mars, Titan, and Venus [PDF]
Valerio Lucarini, Klaus Fraedrich
openalex

