Physics
Scientific paper
Mar 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2847w&link_type=abstract
43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2847
Physics
Scientific paper
The mantle of Mars is in the stagnant lid convection regime where most
of the cold upper boundary layer is immobile and conductive. It is shown
here how crust thickness can influence the thickness and heat flow of
the lid.
No associations
LandOfFree
Stagnant Lid Heterogeneity on Mars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Stagnant Lid Heterogeneity on Mars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stagnant Lid Heterogeneity on Mars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1049208