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GEOPHYSICAL RESEARCH LETTERS, VOL. 33, L21203, DOI:10.1029/2006GL027210, 2006Martian dust storms as a possible sink of atmospheric methane W. M. Farrell,1 G. T. Memory,2 and S. K. Atreya3 Received
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Martian dust storms refer to the swirling clouds of dust that can cover large portions of the Martian surface for weeks or even months.
Scientists and researchers studying Mars are typically the ones required to file reports on martian dust storms.
To fill out a report on martian dust storms, researchers must gather data on the storm's duration, intensity, location, and any impact on the Martian environment.
The purpose of documenting martian dust storms is to better understand the planet's weather patterns and climate, as well as to monitor any changes over time.
Information that must be reported on martian dust storms includes the storm's duration, intensity, location, and any observed impact on the Martian environment.
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