The influence of radiatively active water ice clouds on the Martian climate

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The Modern Near-Surface Martian Climate: A Review of In-situ Meteorological Data from Viking to Curiosity (2017, background): “…contribute to the atmospheric opacity, such as during the aphelion cloud belt or at the edges of the polar caps (Toigo and Richardson 2000; Smith 2004; Madeleine et al. 2012; Lemmon et al. 2015), their effect on the solar insolation at the surface is generally minor compared to that of the dust.”
Martian Year 34 Column Dust Climatology from Mars Climate Sounder Observations: Reconstructed Maps and Model Simulations (2019, methodology): “, 2013), water cycle with radiative effect of clouds (Madeleine et al., 2012) and full microphysics scheme (Navarro et al.”
NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance (2018, background): “…et al. (2004), Mumma et al. (2009). b Fedorova et al. (2008), Smith (2004), Smith et al. (2009a). c Krasnopolsky et al. (1997), Lodders and Fegley (1997), Owen et al. (1977). d Krasnopolsky (2007), Smith et al. (2009b) n Khayat et al. (2015) the formation of clouds (e.g. Madeleine et al. 2012).”
Eight-year climatology of dust optical depth on Mars (2014, background): “A non-exhaustive list of examples includes Guzewich et al. (2013a), Wang and Richardson (2015), Kavulich et al. (2013), Greybush et al. (2012), Madeleine et al. (2011, 2012).”