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Nature communications, 2020-01, Vol.11 (1), p.614-614, Article 614
2020

Details

Autor(en) / Beteiligte
Titel
Dust tides and rapid meridional motions in the Martian atmosphere during major dust storms
Ist Teil von
  • Nature communications, 2020-01, Vol.11 (1), p.614-614, Article 614
Ort / Verlag
England: Nature Publishing Group
Erscheinungsjahr
2020
Link zum Volltext
Quelle
Alma/SFX Local Collection
Beschreibungen/Notizen
  • The atmosphere of Mars is strongly affected by the spatial and temporal variability of airborne dust. However, global dust variability within a sol (Martian day) is still poorly understood. Although short-term dynamic processes are crucial, detailed comparisons of simulated diurnal variations are limited by relatively sparse observations. Here, we report the discovery of ubiquitous, strong diurnal tides of dust in the Southern Hemisphere of Mars. Driven by the westward-propagating migrating diurnal thermal tide, zonally distributed dust fronts slosh back and forth in a wide latitudinal range of up to 40° within one sol during major dust storms. Dust tides-tidal transport of dust in this way-rapidly transport heat and constituents meridionally, allowing moist air near the summer pole to be rapidly transported to lower latitudes during the night, where it then can be lifted by daytime deep convection and contribute to hydrogen escape from Mars during global dust storms.
Sprache
Englisch
Identifikatoren
ISSN: 2041-1723
eISSN: 2041-1723
DOI: 10.1038/s41467-020-14510-x
Titel-ID: cdi_doaj_primary_oai_doaj_org_article_4b5a90ab83b442e391fbed00e4056952

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