Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Samuel Atwood"'
Autor:
Michael Smith, Khalid Badri, Samuel Atwood, Christopher Edwards, Philip Christensen, Michael Wolff
Thermal infrared spectra taken by the Emirates Mars Infrared Spectrometer (EMIRS) enable the retrieval of atmospheric temperature profiles from near the surface to ~40 km, and the column abundance of dust aerosols, water ice clouds, and water vapor.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cdf1a500d886a788e441ba5fa51d5ffb
https://doi.org/10.5194/egusphere-egu23-8786
https://doi.org/10.5194/egusphere-egu23-8786
Background Water vapor in the Martian atmosphere can condense into ice-crystals, forming water ice clouds. At one hand, this works as a cooling mechanism by reflecting incoming solar radiation back into space, and on the other hand as a warming mecha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6f6fd604c79cfb067772c07b16ea2f0b
https://doi.org/10.5194/epsc2022-617
https://doi.org/10.5194/epsc2022-617
Autor:
Siteng Fan, Francois Forget, Michael Smith, Sandrine Guerlet, Khalid Badri, Samuel Atwood, Christopher Edwards, Philip Christensen, Justin Deighan, Hessa Al Matroushi, Antoine Bierjon, Jiandong Liu, Ehouarn Millour
Thermal tides are planetary-scale harmonic responses driven by diurnal solar forcing and influenced by planetary topography. Excited by solar heating absorbed by the atmosphere and energy exchange with surface, thermal tides grow in Martian atmospher
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e134e95cef80b96087e8fa71c3d11993
https://doi.org/10.5194/egusphere-egu22-4208
https://doi.org/10.5194/egusphere-egu22-4208