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Analyzing the development of two regional dust storms on Mars using MRO-MCS and Perseverance observations
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DOI：10.1016/j.aeolia.2025.101010.png)
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Abstract
En 中文
• Instability, zonal to local circulation, topography, and dust supply primarily drive storm growth. • Unstable layers reach a maximum of 25 km, while the latitudinal extent is season-dependent. • Stable layers with bridge like structure form during the expansion phase of the storms. • The storms and the Hadley circulation transport dust up to 25–60 km at various locations. • Jezero crater experiences considerable temperature, pressure, and humidity shifts during the storms.
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