Dust storms on Mars are important weather phenomena that are intricately linked to the dynamics and thermodynamics of the atmosphere. This study utilized the observations from Mars Climate Sounder (MCS) instrument onboard the Mars Reconnaissance Orbiter (MRO) and Mars Environmental Dynamics Analyzer (MEDA) onboard the Perseverance rover, to analyze the growth and development of two regional dust storms occurred in the Martian Year (MY) 36. The said dust storms were observed around LS = 153°–156° (RDS-A) and 310°–330° (RDS-B). MCS observations realized unstable layers in the latitude range 40°S–90°N for RDS-A, and 90°S–40°N for RDS-B, mostly up to 25 km altitude. During the storms’ extension phase, a stable layer with a bridge-like structure forms at 40–60 km for RDS-A and 20–40 km for RDS-B. The mixing ratio values indicated higher availability of dust particles at 30–50 km in 40°S–40°N region for RDS-A and at 25–60 km in 90°S-40°N region for RDS-B. MEDA observations displayed a decrease in daytime ground and air temperature, but an increase during the night. The overall pressure increased during the storm, but the minimum pressure was found to decrease. Pressure variation exhibited the diurnal behavior to the presence of four components. The detection of higher number of vortices during the storms indicated the possibility of the contribution of storm-induced turbulence. The current study provided some insights on the intricate dust-lifting mechanisms, advancing the understanding of the Martian atmosphere.
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