Present-day heat flow model of Mars-Reference-Cited by-同舟云学术

Present-day heat flow model of Mars

Published:2017-04-03 Issue:1 Volume:7 Page:
ISSN:2045-2322
Container-title:Scientific Reports
language:en
Short-container-title:Sci Rep

Author:

Parro Laura M.,Jiménez-Díaz Alberto,Mansilla Federico,Ruiz Javier

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/srep45629.pdf

Reference66 articles.

1. Ruiz, J. The early heat loss evolution of Mars and their implications for internal and environmental history. Sci. Rep. 4, 4338, doi: 10.1038/srep04338 (2014).

2. Spohn, T. et al. InSight: Measuring the Martian Heat Flow using the Heat Flow and Physical Properties Package (HP3). Lunar Planet. Sci. Conf. 43, 1445 (2012).

3. Solomon, S. C. & Head, J. W. Heterogeneities in the thickness of the elastic lithosphere of Mars: Constraints on heat flow and internal dynamics. J. Geophys. Res. 95, 11073–11083 (1990).

4. McGovern, P. J. et al. Localized gravity/topography admittance and correlation spectra on Mars: Implications for regional and global evolution. J. Geophys. Res. 107, 5136, doi: 10.1029/2002JE001854 (2002).

5. McGovern, P. J. et al. Correction to Localized gravity/topography admittance and correlation spectra on Mars: implications for regional and global evolution. J. Geophys. Res. 109, E07007, doi: 10.1029/2004JE002286 (2004).

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