Convection in Enceladus' ice shell: Conditions for initiation

Author:

Barr Amy C.1,McKinnon William B.2

Affiliation:

1. Department of Space Studies; Southwest Research Institute; Boulder Colorado USA

2. Department of Earth and Planetary Sciences and the McDonnell Center for the Space Sciences; Washington University; St. Louis Missouri USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference32 articles.

1. Convection in ice I shells and mantles with self-consistent grain size;Barr;J. Geophys. Res.,2007

2. Onset of convection in the icy Galilean satellites: Influence of rheology;Barr;J. Geophys. Res.,2005

3. Convective instability in ice I with non-Newtonian rheology: Application to the icy Galilean satellites;Barr;J. Geophys. Res.,2004

4. Collins , G. J. C. Goodman 2006 Internal melting and the shape of Enceladus the 38th Annual Meeting of the Division for Planetary Sciences Pasadena, Calif.

5. Rheological properties of water ice-Applications to satellites of the outer planets;Durham;Annu. Rev. Earth Planet. Sci.,2001

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