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- W2605798968 abstract "We calculate the seasonal and interannual variation in dust aerosol particle size above Gale Crater during the first 1413 sols of the Mars Science Laboratory (MSL) mission. Measurements of UV radiation made by the Rover Environmental Monitoring Station (REMS) in combination with atmospheric opacities retrieved from the Mastcam instrument are used for the calculations. Our results indicate that the dust effective radius varies significantly with season, ranging from ~0.6 µm during the low opacity season (Ls = 60° – 140°) to ~2 µm during the high opacity season (Ls = 180° – 360°). Our results suggest that Gale Crater is affected by dust events of high aerosol content originated at various distances from it. Our results improve the accuracy of estimations of ultraviolet radiation fluxes at the Martian surface. Moreover, our results have important implications because the lifetime of suspended dust and its ability to nucleate clouds are affected by particle size." @default.
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- W2605798968 date "2017-04-24" @default.
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- W2605798968 title "Determination of dust aerosol particle size at Gale Crater using REMS UVS and Mastcam measurements" @default.
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- W2605798968 doi "https://doi.org/10.1002/2017gl072589" @default.
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