Literature DB >> 11449286

Weather and climate on Mars.

C Leovy1.   

Abstract

Imagine a planet very much like the Earth, with similar size, rotation rate and inclination of rotation axis, possessing an atmosphere and a solid surface, but lacking oceans and dense clouds of liquid water. We might expect such a desert planet to be dominated by large variations in day-night and winter-summer weather. Dust storms would be common. Observations and simulations of martian climate confirm these expectations and provide a wealth of detail that can help resolve problems of climate evolution.

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Year:  2001        PMID: 11449286     DOI: 10.1038/35084192

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


  2 in total

1.  Snowball Earth climate dynamics and Cryogenian geology-geobiology.

Authors:  Paul F Hoffman; Dorian S Abbot; Yosef Ashkenazy; Douglas I Benn; Jochen J Brocks; Phoebe A Cohen; Grant M Cox; Jessica R Creveling; Yannick Donnadieu; Douglas H Erwin; Ian J Fairchild; David Ferreira; Jason C Goodman; Galen P Halverson; Malte F Jansen; Guillaume Le Hir; Gordon D Love; Francis A Macdonald; Adam C Maloof; Camille A Partin; Gilles Ramstein; Brian E J Rose; Catherine V Rose; Peter M Sadler; Eli Tziperman; Aiko Voigt; Stephen G Warren
Journal:  Sci Adv       Date:  2017-11-08       Impact factor: 14.136

2.  Dust tides and rapid meridional motions in the Martian atmosphere during major dust storms.

Authors:  Zhaopeng Wu; Tao Li; Xi Zhang; Jing Li; Jun Cui
Journal:  Nat Commun       Date:  2020-01-30       Impact factor: 14.919

  2 in total

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