Results 161 to 170 of about 736,131 (304)

Dual-Wavelength Interferometric Detection Technology for Wind and Temperature Fields in the Martian Middle and Upper Atmosphere Based on LCTF

Remote Sensing
A dual-wavelength spaceborne Martian polarized wind imaging Michelson interferometer based on liquid crystal tunable filters (LCTF-MPWIMI) has been proposed for the remote sensing detection of dynamic parameters such as wind speed and temperature in the ...
Yanqiang Wang, Biyun Zhang, Chunmin Zhang, Shiping Guo, Tingyu Yan, Yifan He, William Ward   +6 more
doaj   +1 more source

A new perspective on gravity waves in the Martian atmosphere: Sources and features [PDF]

, 2011
Yoshizumi Miyoshi, J. M. Forbes, Y. Moudden   +2 more
openalex   +1 more source

The Martian Atmosphere During the Viking Mission, I Infrared Measurements of Atmospheric Temperatures Revisited

, 2000
R. J. Wilson
openalex   +2 more sources

Martian Dust Storms and Gravity Waves: Disentangling Water Transport to the Upper Atmosphere

, 2021
Dmitry S. Shaposhnikov, Alexander S. Medvedev, A. V. Rodin, Erdal Yiğit, P. Hartogh   +4 more
openalex   +3 more sources

On the strong and selective isotope effect in the UV excitation of N ₂ with implications toward the nebula and Martian atmosphere

, 2011
B. H. Muskatel, F. Remacle, M. H. Thiemens, R. D. Levine   +3 more
openalex   +2 more sources

Martian Surface and Atmosphere Workshop

Eos, Transactions American Geophysical Union, 1992
The NASA‐sponsored Martian Surface and Atmosphere Through Time Study Project convened its first major meeting at the University of Colorado in Boulder, September 23–25, 1991. The workshop, co‐sponsored by the Lunar and Planetary Institute (LPI) and the Laboratory for Atmospheric and Space Physics at the University of Colorado, brought together an ...
openaire   +1 more source

Ice or liquid water in the Martian regolith. Morphologic indicators from rampart craters [PDF]

The morphology of ejecta blankets around certain Martian craters carries implications for volatiles in either the Martian crust or the atmosphere or both. The evidence that rampart crater ejecta can be used to infer the physical condition of volatiles in
Mouginismark, P. J.
core   +1 more source

The long winter model of Martian biology: A speculation [PDF]

An estimated mean thickness of about 1 km of frost in the Martian north polar cap summer remnant, if vaporized, would yield about 1000 g/sq cm of atmosphere over the planet, higher global temperatures through the greenhouse effect, and a greatly ...
Sagan, C.
core   +1 more source

A Case Study on the Impact of Interplanetary Coronal Mass Ejection on the Martian O(1S) 557.7 nm Dayglow Emission Using ExoMars TGO/NOMAD‐UVIS Observations: First Results

Geophysical Research Letters
We report, for the first time, the impact of interplanetary coronal mass ejections (ICME) on the recently discovered O(1S) 557.7 nm dayglow emission in the Martian atmosphere.
Aadarsh Raj Sharma, Lot Ram, Harshaa Suhaag, Dipjyoti Patgiri, Lauriane Soret, Jean‐Claude Gérard, Ian R. Thomas, Ann Carine Vandaele, Sumanta Sarkhel   +8 more
doaj   +1 more source

Aeolian abrasion of rocks as a mechanism to produce methane in the Martian atmosphere. [PDF]

Sci Rep, 2019
Safi E, Telling J, Parnell J, Chojnacki M, Patel MR, Realff J, Blamey NJF, Payler S, Cockell CS, Davies L, Boothroyd IM, Worrall F, Wadham JL.   +12 more
europepmc   +1 more source