Magma-cryosphere interactions on Mars : the influence of heat-transfer mechanisms on surface morphology
Mars is thought to have a planet-wide cryosphere of several kilometres depth consisting of a mixture of rock and permanently frozen ice. The physical processes occurring during magma-cryosphere interaction (MCI) appear to have played a large part in the morphological development of many regions of M...
Main Author: | Tyson, Shelly |
---|---|
Published: |
Lancaster University
2016
|
Subjects: | |
Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.727389 |
Similar Items
-
Modelling the ultraviolet environment at the surface of Mars and design of the Beagle 2 UV sensor
by: Patel, Manish R.
Published: (2003) -
Studies of glacial and periglacial environments on Mars
by: Ramsdale, Jason
Published: (2017) -
The Beagle 2 X-ray spectrometer for Mars
by: Talboys, Dean Lee
Published: (2006) -
Remote sounding of the Martian atmosphere with Mars climate sounder
by: Adlen, Samuel John Morris
Published: (2004) -
Novel X-ray diffraction and the remote analysis of Mars
by: Turner, Stuart Matthew Robert
Published: (2017)