3:30 PM - 5:00 PM
[PPS05-P14] Mid-latitude disturbances in the Martian atmosphere studied with MRO MCS data
Keywords:Mars, Atmosphere, Atmospheric Dynamics
We have examined the behavior of the waves using Mars Reconnaissance Orbiter (MRO) Mars Climate Sounder (MCS) limb observations data. The retrieved data of temperature, dust, and water ice within a pressure range from 200 to 1 Pa, corresponding to the altitude range from about 10 to 55 km above surface, are used in our analysis. We focused on the mid-to high-latitudes in the northern hemisphere, since the baroclinic waves appear more strongly than in the southern hemisphere. Temperature fluctuations are analyzed after dividing the data into time intervals with a length of 1 Martian day and subtracting the seasonal trend. This makes it possible to see the propagation of the waves with a time resolution of 1 Martian day. Then, we have investigated how the meridional distribution of the wave amplitude changes with time.
In the future, we will examine how the baroclinic waves have an influence on the dust and water ice transportation in high altitudes.