Internal Structure and Mechanisms of Core Convection on Ganymede

Details Internal Structure and Mechanisms of Core Convection on Ganymede Internal Structure and Mechanisms of Core Convection on Ganymede

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1380h&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1380

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Scientific paper

We model Ganymede's non-ice interior to better constrain the conditions
that can lead to internal magnetic field generation. Compositional core
convection can be driven by means other than solid inner core growth.

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