T. Siili

TL;DR: Higher abundances of chlorinated hydrocarbons in the mudstone compared with Rocknest windblown materials previously analyzed by Curiosity suggest that indigenous martian or meteoritic organic carbon sources may be preserved in the Mudstone; however, the carbon source for the chlorinatedHydrocarbons is not definitively of martian origin.

TL;DR: The planetary boundary layer (PBL) represents the part of the atmosphere that is strongly influenced by the presence of the underlying surface and mediates the key interactions between the atmosphere and the surface as mentioned in this paper.

TL;DR: The REMS-H measurement performance and initial observations during the first 100 MSL sols appear to be convincing and are aligned with earlier indirect observations of the total atmospheric precipitable water content.

TL;DR: In this paper, the summertime Martian PBL diurnal wind variation, slope winds, and the nocturnal low-level jets were studied using Prandtl's theory, a mesoscale numerical model, and Viking lander observations.

TL;DR: In this paper, the pressure measurement subsystem of the Mars Science Laboratory (MSL) Rover Environmental Measurement Station (REMS-P) performed accurate observations of the Martian atmospheric surface pressure.