How large are present-day heat flux variations across the surface of Mars?-Reference-Cited by-同舟云学术

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How large are present-day heat flux variations across the surface of Mars?

Published:2016-12 Issue:12 Volume:121 Page:2386-2403
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Plesa A.-C.¹,Grott M.¹,Tosi N.¹²,Breuer D.¹,Spohn T.¹,Wieczorek M. A.³^ORCID

Affiliation:

1. German Aerospace Center (DLR); Berlin Germany

2. Department of Astronomy and Astrophysics; Technische Universität Berlin; Berlin Germany

3. Institut de Physique du Globe de Paris, Sorbonne Paris Cité; Paris VII - Denis Diderot University; Paris France

Funder

Interuniversity Attraction Poles Programme initiated by the Belgian Science Policy Office through the Planet TOPERS alliance

Helmholtz-Gemeinschaft

HLRN

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2016JE005126/fullpdf

Reference73 articles.

1. The Borealis basin and the origin of the Martian crustal dichotomy;Andrews-Hanna;Nature,2008

2. Petrological constraints on the density of the Martian crust;Baratoux;J. Geophys. Res. Planets,2014

3. Constraints on the Martian lithosphere from gravity and topography data;Belleguic;J. Geophys. Res.,2005

4. Three dimensional models of Martian mantle convection with phase transitions;Breuer;Geophys. Res. Lett.,1998

5. The effective elastic thickness (Te) of continental lithosphere: What does it really mean?;Burov;J. Geophys. Res.,1995

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