Constraints on the formation and properties of a Martian lobate debris apron: Insights from high-resolution topography, SHARAD radar data, and a numerical ice flow model-Reference-Cited by-同舟云学术

Constraints on the formation and properties of a Martian lobate debris apron: Insights from high-resolution topography, SHARAD radar data, and a numerical ice flow model

Published:2016-03 Issue:3 Volume:121 Page:432-453
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Parsons Reid¹,Holt John²

Affiliation:

1. Department of Earth and Geographic Sciences; Fitchburg State University; Fitchburg Massachusetts USA

2. Institute for Geophysics and Department of Geological Sciences, Jackson School of Geosciences; University of Texas at Austin; Austin Texas USA

Funder

NASA Mars Data Analysis Program

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference91 articles.

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2. Grain growth in polar ice. II;Alley;J. Glaciol.,1986

3. Flow patterns of lobate debris aprons and lineated valley fill north of Ismeniae Fossae, Mars: Evidence for extensive mid-latitude glaciation in the Late Amazonian;Baker;Icarus,2010

4. Observations of polar ice from the Holocene and the glacial period using the scanning electron microscope;Barnes;Ann. Glaciol.,2002

5. Ice grain size and rheology of the Martian polar deposits;Barr;Icarus,2008

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