Results 101 to 110 of about 53,886 (238)

The utilization of powdered metals as fuels in the atmospheres of Venus, Earth, and Mars [PDF]

Ignition temperatures of powdered metals in simulated Mars and Venus ...
Rhein, R. A.
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Altitude Profile and Isotopic Composition for N2 From Pioneer Venus Mass Spectra

Geophysical Research Letters
We report the highest resolution altitude profile and isotopic composition for N2 at Venus, to date. These results were obtained through re‐analysis of data acquired by the Pioneer Venus Large Probe Neutral Mass Spectrometer (LNMS).
R. Mogul, S. S. Limaye, M. J. Way
doaj   +1 more source

Sudy of the Propagation of Decimeter Radiowaves in the Atmosphere of Venus with the Aid of AIS ''venera 4'' [PDF]

Radio wave propagation in Venus atmosphere based on approximating inhomogeneity of ...
Kolosov, M. A., Yakovlev, O. I., Yefimov, A. I.   +2 more
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Calculations of the Radiative and Dynamical State of the Venus Atmosphere [PDF]

, 1975
James B. Pollack, Richard E. Young
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Effective parameterization of absorption by gaseous species and unknown UV absorber in 125–400 nm region of Venus atmosphere [PDF]

, 2022
B. A. Fomin, Mikhail Razumovskiy
openalex   +1 more source

The impacts of coronal mass ejections on the space environments of Venus and Mars

地球与行星物理论评
Coronal mass ejections (CME) are solar transients, and their impacts on the planets within the solar system have attracted considerable attention. As neighboring planets within the solar system, Venus and Mars are also directly and indirectly affected by
Qi Xu, Lianghai Xie, Lei Li, Xiaojun Xu
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Long-term variations in abundance and distribution of sulfuric acid vapor in the Venus atmosphere inferred from Pioneer Venus and Magellan radio occultation studies [PDF]

Radio occultation experiments have been used to study various properties of planetary atmospheres, including pressure and temperature profiles, and the abundance profiles of absorbing constituents in those planetary atmospheres. However, the reduction of
Jenkins, J. M., Steffes, P. G.
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Life on Venus?

Life
Venus is not generally at the forefront when considering extraterrestrial life. Yet, based on the physical similarities and proximity to Earth and with the little knowledge of its evolutionary history, there is a possibility that Venus may have hosted ...
Sanjay S. Limaye
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Origin and early evolution of terrestrial planet atmospheres and oceans

Terrestrial, Atmospheric and Oceanic Sciences, 2019
Planet atmospheric compositions are determined by the availability of a gas species, its molecular weight and the mass (or gravity force) of a planet. Both Mercury and the Moon are not massive enough to hold any gas species to form an atmosphere.
Lin-gun Liu
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General circulation in the atmosphere of Venus driven by polar and diurnal variations of surface temperature [PDF]

Mathematical model for Venus atmosphere circulation pattern determined by polar and diurnal temperature ...
Bohachevsky, I. O., Yeh, T. T. J.
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