The impact of martian mesoscale winds on surface temperature and on the determination of thermal inertia
Radiative control of surface temperature is a key characteristic of the martian environment and its low-density atmosphere. Here we show through meteorological modeling that surface temperature can be far from radiative equilibrium over numerous sloping terrains on Mars, where nighttime mesoscale ka...
Asıl Yazarlar: | Spiga, A, Forget, F, Madeleine, J, Montabone, L, Lewis, SR, Millour, E |
---|---|
Materyal Türü: | Journal article |
Dil: | English |
Baskı/Yayın Bilgisi: |
2011
|
Benzer Materyaller
-
Influence of water ice clouds on Martian tropical atmospheric temperatures
Yazar:: Wilson, R, ve diğerleri
Baskı/Yayın Bilgisi: (2008) -
Assimilating and modeling dust transport in the martian climate system
Yazar:: Ruan, T, ve diğerleri
Baskı/Yayın Bilgisi: (2012) -
Revisiting the radiative impact of dust on Mars using the LMD Global Climate Model
Yazar:: Madeleine, J, ve diğerleri
Baskı/Yayın Bilgisi: (2011) -
Interannual variability of Martian dust storms in assimilation of several years of Mars global surveyor observations
Yazar:: Montabone, L, ve diğerleri
Baskı/Yayın Bilgisi: (2005) -
Validation of martian meteorological data assimilation for MGS/TES using radio occultation measurements
Yazar:: Montabone, L, ve diğerleri
Baskı/Yayın Bilgisi: (2006)