Zobrazeno 1 - 10
of 144
pro vyhledávání: '"Robert M. Haberle"'
Humanity has long been fascinated by the planet Mars. Was its climate ever conducive to life? What is the atmosphere like today and why did it change so dramatically over time? Eleven spacecraft have successfully flown to Mars since the Viking missio
Publikováno v:
Icarus. 394:115401
Autor:
Robert M. Haberle
The climate of Mars has evolved over time. Early in its history, between 3.7 and 4.1 billion years ago, the climate was warmer and wetter and the atmosphere thicker than it is today. Erosion rates were higher than today, and liquid water flowed on th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5d40950d6da7dbd6b6384c2346ae5687
https://doi.org/10.1093/acrefore/9780190647926.013.122
https://doi.org/10.1093/acrefore/9780190647926.013.122
Publikováno v:
The Astrophysical Journal. 941:54
The dust cycle is the dominant driver of meteorology and climate on present-day Mars. Despite this, few studies have investigated the impact of dust interacting with incoming stellar radiation on the climate, habitability, and potential spectral sign
Publikováno v:
Geophysical Research Letters. 46:13355-13362
Publikováno v:
Icarus. 330:169-188
The nature of the early Martian climate has been the subject of debate for decades, with geologic evidence suggesting an environment with prolonged precipitation and flowing liquid water on the surface, while climate models have struggled to reproduc
Autor:
David M. Kass, Manuel de la Torre Juárez, Jeffrey R. Barnes, Henrik Kahanpää, Ari-Matti Harri, Melinda A. Kahre, Robert M. Haberle, Jeffery L. Hollingsworth
Publikováno v:
Icarus. 307:150-160
The Rover Environmental Monitoring Station (REMS) on the Curiosity Rover is operating in the Southern Hemisphere of Mars and is detecting synoptic period oscillations in the pressure data that we attribute to Northern Hemisphere transient eddies. We
Autor:
Michael J. Wolff, Robert M. Haberle, R. John Wilson, Jeffery L. Hollingsworth, Melinda A. Kahre, Amanda Brecht, J. Schaeffer, Richard A. Urata, Alexandre Kling, Franck Montmessin
Publikováno v:
Icarus
Icarus, Elsevier, 2019, 333, pp.130-164. ⟨10.1016/j.icarus.2019.03.026⟩
Icarus, Elsevier, 2019, 333, pp.130-164. ⟨10.1016/j.icarus.2019.03.026⟩
International audience; We describe and document the physics packages in the legacy NASA/Ames Mars Global Climate Model, present simulations of the seasonal water cycle and how it compares with observations, assess the role of radiatively active clou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1185591bc147eae8432a2046264c96e
https://hal-insu.archives-ouvertes.fr/insu-02107018/document
https://hal-insu.archives-ouvertes.fr/insu-02107018/document
Autor:
Melinda A. Kahre, Michael J. Wolff, Robert M. Haberle, R. Todd Clancy, Bruce A. Cantor, François Forget, Michael C. Malin
Publikováno v:
Icarus
Icarus, Elsevier, 2019, 332, pp.24-49. ⟨10.1016/j.icarus.2019.05.041⟩
Icarus, Elsevier, 2019, 332, pp.24-49. ⟨10.1016/j.icarus.2019.05.041⟩
Observations by the Mars Color Imager (MARCI) onboard the Mars Reconnaissance Orbiter (MRO) in the ultraviolet (UV, Band 7; 320 nm) are used to characterize the spatial and temporal behavior of atmospheric water ice over a period of 6 Mars Years. Exp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::411bc6bde0b612529c7e13b54f49cd78
https://hal.archives-ouvertes.fr/hal-03104116
https://hal.archives-ouvertes.fr/hal-03104116
Autor:
Frances Rivera-Hernandez, Robert M. Haberle, Alexandre Kling, Christopher P. McKay, Thomas F. Bristow
Sedimentary deposits characterized by the Mars Science Laboratory Curiosity rover provide evidence that Gale crater, Mars intermittently hosted a fluvio-lacustrine environment during the Hesperian. However, estimates of the CO2 content of the atmosph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e884c8d899765468dcc17f6a22f4062