Density and temperatures of the upper Martian atmosphere measured by stellar occultations with Mars Express SPICAM

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Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere (2015, methodology): “, 2006] in order to improve the calculation of Mars mesopause temperatures and heights [Forget et al., 2009; McDunn et al., 2010].”
Structure and dynamics of the Martian lower and middle atmosphere as observed by the Mars Climate Sounder: Seasonal variations in zonal mean temperature, dust, and water ice aerosols (2010, unknown): “…spectroscopy [Smith et al., 2001; Smith, 2004], from which an extensive climatology has been developed, and radio occultation [Hinson et al., 2004], and measurements in the upper atmosphere obtained from aerobraking experiments [Keating et al., 1998], and stellar occultation [Forget et al., 2009].”
Three‐dimensional Martian ionosphere model: I. The photochemical ionosphere below 180 km (2013, result): “, 2011], this indicates that the model reproduces correctly the temperatures in the Martian mesosphere/mesopause/lower thermosphere region, in contrast with previous results [Forget et al., 2009; González-Galindo et al., 2009].”