Frozen Martian lahars? Evaluation of morphology, degradation and geologic development in the Utopia–Elysium transition zone
- 1 September 2013
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 85, 59-77
Abstract
No abstract availableKeywords
Funding Information
- Forskerakademiet
This publication has 48 references indexed in Scilit:
- Elysium‐Utopia flows as mega‐lahars: A model of dike intrusion, cryosphere cracking, and water‐sediment releaseJournal of Geophysical Research, 2003
- Geomorphic analysis of lobate debris aprons on Mars at Mars Orbiter Camera scale: Evidence for ice sublimation initiated by fracturesJournal of Geophysical Research, 2003
- Topographic analysis of features related to ice on MarsGeophysical Research Letters, 2001
- Kilometer‐scale roughness of Mars: Results from MOLA data analysisJournal of Geophysical Research, 2000
- Magmatic intrusions and a hydrothermal origin for fluvial valleys on MarsJournal of Geophysical Research, 1998
- The enormous Chillos Valley Lahar: an ash-flow-generated debris flow from Cotopaxi Volcano, EcuadorBulletin of Volcanology, 1998
- Mars: Review and analysis of volcanic eruption theory and relationships to observed landformsReviews of Geophysics, 1994
- Volcanic influences on terrestrial sedimentationGeology, 1989
- The evolution of lava flow-fields: observations of the 1981 and 1983 eruptions of Mount Etna, SicilyBulletin of Volcanology, 1987
- Large volcanic debris avalanches: Characteristics of source areas, deposits, and associated eruptionsJournal of Volcanology and Geothermal Research, 1984