Article ID Journal Published Year Pages File Type
1773919 Icarus 2012 7 Pages PDF
Abstract
► We measure zonal wind velocities in the martian mesosphere by infrared spectroscopy. ► IR ground based observations provide spatial resolution. ► GCM predictions from the Mars Climate Database are mostly consistent with the observations.
Keywords
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
Preview
Mars mesospheric zonal wind around northern spring equinox from infrared heterodyne observations of CO2
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