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

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Global climate modeling of the Martian water cycle with improved microphysics and radiatively active water ice clouds (2013, background): “In particular, it has been suggested that scavenging could explain the formation of the detached dust layers observed by Mars Climate Sounder [ McCleese et al. , 2010; Heavens et al. , 2011a] by the enrichment of dust below the ice clouds (by releasing the dust when the cloud sublimates) or by…”
Eight-year climatology of dust optical depth on Mars (2014, background): “12 and 13 of McCleese et al., 2010, give an idea of the diurnal variability of the dust extinction profile).”
Ice structures, patterns, and processes: A view across the icefields (2012, background): “The polar regions of Mars are rich in ices (mainly carbon dioxide and water), but frozen aerosols containing these species 13 are also detected in the Martian stratosphere (McCleese et al., 2010).”