The onset and growth of the 2018 Martian Global Dust Storm

Abstract

We analyze the onset and initial expansion of the 2018 Martian Global Dust Storm (GDS 2018) using ground-based images in the visual range. This is the first case of a confirmed GDS initiating in the Northern Hemisphere. A dusty area extending about 1.4x10e5 km^2 and centered at latitude +31.7° $\pm$ 1.8° and west longitude 18° $\pm$ 5°W in Acidalia Planitia was captured on 30 and 31 May 2018 (Ls = 184.9°). From 1 to 8 June, daily image series showed the storm expanding southwards along the Acidalia corridor with velocities of 5 m/s, and simultaneously progressing eastwards and westwards with horizontal velocities ranging from 5 to 40 m/s. By 8 June the dust reached latitude -55° and later penetrated in the South polar region, whereas in the North the dust progression stopped at latitude +46°. We compare the onset and expansion stage of this GDS with the previous confirmed storms.

Accepted in Geophysical Research Letters. Main article and Supporting Information

References in corpus (1)

• The 2018 Martian Global Dust Storm over the South Polar Region studied with MEx/VMC

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