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Hellas and dust storms on Mars. [Mechanism, wind velocity]

Journal Article · · Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:7352754
The development of slope winds in the round Hellas basin can generate an anticyclone during (and only during) the summer-solstice period in the southern hemisphere of Mars. The wind velocity at the periphery of the anticyclone would be sufficient to initiate a global dust storm. This mechanism might account for the timing of global storms at Martian perihelion and for the tendency of storms to commence in the neighborhood of Hellas.
Research Organization:
Astronomical Council, Moscow
OSTI ID:
7352754
Journal Information:
Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 1:1; ISSN SALED
Country of Publication:
United States
Language:
English

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