Results 91 to 100 of about 4,918 (242)

The Dominant Role of Crustal Fields in Structuring Electromagnetic Environment Within the Martian Dayside Magnetosphere

Geophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract Although Mars lacks an intrinsic global dipole magnetic field, the existence of crustal magnetic anomalies in the southern hemisphere causes the Martian magnetosphere to have the hybrid characteristics combining Venus‐like induced and Earth‐like intrinsic types.
Shibang Li, Haoyu Lu, Jinbin Cao, Nihan Chen, Yihui Song, Jianxuan Wang, Yuchen Cao, Jianing Zhao, Qimeng Wang   +8 more
wiley   +1 more source

Aerial Platforms for Exploration Under Extreme Conditions in the Venus Atmosphere

RUDN Journal of Engineering Research
This paper explores various aerial platforms for in-situ atmospheric exploration of Venus, emphasizing their potential integration into future missions.
Victor A. Vorontsov, Michael V. Quispe Mendoza   +1 more
doaj   +1 more source

Remote sensing of planetary atmospheres: Venus

Advances in Space Research, 1998
Abstract More than any other planet except the Earth, Venus has been the subject of a variety of remote sensing investigations over a wide range of wavelengths. Since Venus has complete cloud cover, with a complex composition and layering, the retrieval of the information from these measurements is particularly challenging.
openaire   +2 more sources

Plasma Acceleration by Magnetic Tension Forces in the Martian Magnetotail: MAVEN Observations

Geophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract The Martian magnetotail is a dynamic region where several processes contribute to plasma acceleration. Here, we analyze ∼5 ${\sim} 5$ years of Mars Atmosphere and Volatile EvolutioN (MAVEN) data to evaluate the role of magnetic tension forces in driving plasma acceleration within current sheets in the tail. Based on magnetic field measurements,
Norberto Romanelli, Ronan Modolo, Gina A. DiBraccio, Jacob R. Gruesbeck, Shaosui Xu, Christopher M. Fowler, Eduard Dubinin, Jasper S. Halekas, Shannon M. Curry, Robert J. Lillis, Jared R. Espley, Kathleen G. Hanley, Yingjuan Ma, Suranga Ruhunusiri, David L. Mitchell, Christian Mazelle   +15 more
wiley   +1 more source

Microwave Opacity of the Venus Atmosphere

The Astronomical Journal, 1969
Surface dielectric constant and microwave opacity of Venus atmosphere as function of wavelength determined by radar ...
openaire   +1 more source

Three Worlds in One: Venus as a Natural Laboratory for the Effect of Rotation Period on Atmospheric Circulation

The Astrophysical Journal Letters
Because of its rotation period of 243 days, Venus is considered a slowly rotating planet. However, its persistent superrotating atmospheric jets, which increase in speed from surface to cloud tops, effectively set a faster rotation speed than the surface
Maureen Cohen, James Holmes, Stephen Lewis, Manish Patel, Sébastien Lebonnois   +4 more
doaj   +1 more source

Chemical Analysis of Materials Exposed to Venus Temperature and Surface Atmosphere [PDF]

, 2018
Dorothy Lukco, David J. Spry, R. P. Harvey, Gustavo Costa, Robert S. Okojie, Amir Avishai, Leah M. Nakley, Philip G. Neudeck, Gary W. Hunter   +8 more
openalex   +1 more source

Net exchange parameterization of thermal infrared radiative transfer in Venus' atmosphere [PDF]

, 2009
V. Eymet, Richard Fournier, Jean‐Louis Dufresne, S. Lebonnois, F. Hourdin, M. A. Bullock   +5 more
openalex   +1 more source

Frequency Channel Selection and Performance Simulation of a Microwave Radiometer for Temperature and Sulfuric Compound Profiling of the Venusian Lower Atmosphere

Earth and Space Science
Exploring the Venusian lower atmosphere is crucial for studying the atmospheric circulation, surface‐atmosphere interactions, and origin and evolution of the Venusian atmosphere and climate. In this study, we investigate the theoretical capabilities of a
Zijin Zhang, Xiaolong Dong, Jian Xu, Jieying He, Wenyu Wang   +4 more
doaj   +1 more source

Abiotic ozone in the observable atmospheres of Venus and Venus-like exoplanets

Monthly Notices of the Royal Astronomical Society
ABSTRACT Ozone is a potential biosignature and disambuguator between Earth-like and Venus-like exoplanets due to its association on Earth with photosynthetically produced oxygen (O$_2$). However, the existence of ozone in Venus’s observable atmosphere, a planet with no known life, raises the possibility of ozone biosignature false ...
Robb Calder, Oliver Shorttle, Sean Jordan, Paul Rimmer, Tereza Constantinou   +4 more
openaire   +3 more sources