共 63 条
- [1] Hartogh P.(2005)escription and climatology of a new general circulation model of the Martian atmosphere J. Geophys. Res. 110 E11008-144
- [2] Medvedev A.S.(2014)Reliable infrared line lists for 13 CO J. Quant. Spectrosc. Radiat. Transf. 147 134-998
- [3] Kuroda T.(2011) isotopologues up to Planet. Space Sci. 59 988-1009
- [4] Saito R.(2011)' = 18,000 cm Planet. Space Sci. 59 999-266
- [5] Villanueva G.(2013) and 1500 K, with line shape parameters Science 341 263-30
- [6] Feofilov A.G.(2003)Modeling the atmospheric limb emission of CO Solar Syst. Res. 37 20-73
- [7] Kutepov A.A.(2015) at 4.3 µm in the terrestrial planets J. Quant. Spectrosc. Radiat. Transf. 152 45-25916
- [8] Berger U. D.(1996)Modelling the atmospheric CO J. Geophys. Res. D 101 25897-263
- [9] Huang X.(2013) 10-µm non-thermal emission in Mars and Venus at high spectral resolution Science 341 260-undefined
- [10] Gamache R.R.(undefined)MSL Science Team, Abundance and isotopic composition of gases in the Martian atmosphere from the Curiosity rover undefined undefined undefined-undefined