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Mars Weather Analysis from Sol 1 to 200: Pressure, Temperature, Vortex Detection

Explore the pressure variation, temperature evolution, and Vortex detection on Mars from the beginning of the mission up to 200 Sols. The data from air and ground temperature sensors reveal the ambient temperature changes. Discover whirlwind signatures through pressure, wind, and ultraviolet radiation parameters. Analyze the relative humidity variations in the Martian atmosphere.

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Mars Weather Analysis from Sol 1 to 200: Pressure, Temperature, Vortex Detection

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  1. Pressure variation from the beginning of the mission

  2. MAX-MIN. TEMPERATURE EVOLUTION Air and ground temperature sensors shows the evolution of the ambient temperature along the first 200 sols.

  3. VORTEX DETECTED BY REMS Vortices are phenomena seen by previous missions. Pressure, wind and ultraviolet radiation are parameters that show whirlwind signatures.

  4. ATMOSPHERE RELATIVE HUMIDITY Relative humidity shows variations from first sols to the actual position.

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