Results 131 to 140 of about 35,859 (291)

Characteristics of the Martian atmosphere surface layer [PDF]

Elements of various terrestrial boundary layer models are extended to Mars in order to estimate sensible heat, latent heat, and momentum fluxes within the Martian atmospheric surface ('constant flux') layer.
Clow, G. D., Haberle, R. M.
core   +1 more source

Thermal Infrared Spectrometers for the Polar Radiant Energy in the Far‐Infrared Experiment (PREFIRE)

Earth and Space Science, Volume 12, Issue 10, October 2025.
Abstract The Polar Radiant Energy in the Far‐InfraRed Experiment (PREFIRE) was selected by NASA to fly two miniaturized Thermal InfraRed Spectrometers (TIRS) capable of distinguishing the spectral signatures of surface and atmospheric properties in Earth's polar regions.
Brian J. Drouin, Tristan L’Ecuyer, Sharmila Padmanabhan, Marc Foote, Rudi Bendig, Simon Calcutt, Gary Hawkins, Harrison Herzog, Eric Hochberg, Matthew Kenyon, Giacomo Mariani, David A. Martinez, James McGuire, Ian Mckinley, Aronne Merrelli, Deacon Nemchick, Nasrat Raouf, Gary Spiers, Daniel Wilson   +18 more
wiley   +1 more source

What martian meteorites reveal about the interior and surface of Mars

, 2020
Arya Udry, Geoffrey H. Howarth, C. D. K. Herd, James M.D. Day, T. J. Lapen, J. Filiberto   +5 more
openalex   +2 more sources

Regional Ice‐Depth and Thickness in Phlegra Montes, Mars From Radar Characterization of Glacial Landsystems Using SHARAD

Journal of Geophysical Research: Planets, Volume 130, Issue 10, October 2025.
Abstract Morphological analyses of Viscous Flow Features (VFFs) in the mid‐latitude regions of Mars have led to the hypothesis that these landforms are equivalent to debris‐covered glaciers. Phlegra Montes is a 1400‐km‐long mountain range in the northern mid‐latitudes that spans from 30° to 50°N, where there is an abundance of glacial landsystems ...
Chimira N. Andres, Isaac B. Smith
wiley   +1 more source

Comparison of Martian surface ionizing radiation measurements from MSL‐RAD with Badhwar‐O'Neill 2011/HZETRN model calculations [PDF]

, 2014
Myung‐Hee Y. Kim, Francis A. Cucinotta, Hatem N. Nounu, C. Zeitlin, Donald M. Hassler, Scot Rafkin, R. F. Wimmer‐Schweingruber, Bent Ehresmann, D. E. Brinza, S. Böttcher, Eckart Böhm, Söenke Burmeister, Jingnan Guo, Jan Köhler, César Martı́n, G. Reitz, A. Posner, Javier Gómez‐Elvira, Ari‐Matti Harri   +18 more
openalex   +1 more source

. . . and martian surfaces [PDF]

Nature, 1989
openaire   +2 more sources

Reconstructing the Early Flow and Deposition Geometry Through the Accretion Surfaces on the Jezero Western Delta Fan, Mars

Journal of Geophysical Research: Planets, Volume 130, Issue 10, October 2025.
Abstract The western delta fan in Jezero crater hosts one of Mars's best‐preserved examples of fluvial accretion surfaces, recently investigated by NASA's Perseverance Rover. Erosional windows reveal this geologic unit, which records evidence of fluvial point bar deposition.
Kartikeya S. Sangwan, Joel M. Davis, Ekta Aggarwal   +2 more
wiley   +1 more source

A model to calculate solar radiation fluxes on the Martian surface [PDF]

, 2015
Á. Vicente‐Retortillo, Francisco P. J. Valero, Luis Vázquez, Germán Martínez   +3 more
openalex   +1 more source

Phase Boundaries Among Three Hydrous Ferric Sulfates and Their Implications for Mars

Journal of Geophysical Research: Planets, Volume 130, Issue 10, October 2025.
Abstract Ferric sulfate minerals have been identified by orbital and landed missions at multiple locations on Mars and are the most common minerals in the Acid Mine Drainage (AMD) system on Earth. The occurrences and the speciation of ferric sulfates are very sensitive to variations in environmental conditions, such as temperature (T), relative ...
Erbin Shi, Alian Wang, I‐Ming Chou, Zongcheng Ling   +3 more
wiley   +1 more source

A DTA/GC for the in Situ Identification of the Martian Surface Material [PDF]

The composition and mineralogy of the Martian surface material remain largely unknown. To determine its composition and mineralogy, several techniques are being considered for in situ analyses of the Martian surface material during missions to Mars.
Mancinelli, R. L., Orenberg, J. B., White, M. R.   +2 more
core   +1 more source