Formation of recurring slope lineae by liquid brines on present-day Mars
Version of Record online: 10 NOV 2012
©2012. American Geophysical Union. All Rights Reserved.
Geophysical Research Letters
Volume 39, Issue 21, November 2012
How to Cite
2012), Formation of recurring slope lineae by liquid brines on present-day Mars, Geophys. Res. Lett., 39, L21202, doi:10.1029/2012GL054119., and (
- Issue online: 10 NOV 2012
- Version of Record online: 10 NOV 2012
- Manuscript Accepted: 5 OCT 2012
- Manuscript Received: 4 OCT 2012
Auxiliary material for this article contains a text file and three figures that describe the model used to calculate the subsurface temperatures.
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Additional file information is provided in the readme.txt.
|grl29763-sup-0001-readme.txt||plain text document||2K||readme.txt|
|grl29763-sup-0002-fs01.tif||TIFF image||728K||Figure S1. Modeled temperatures of surface and shallow subsurface as a function of slope and latitude.|
|grl29763-sup-0003-fs02.tif||TIFF image||22K||Figure S2. Summary of parameters used in the various equations describing the thermal and mass transfer models.|
|grl29763-sup-0004-fs03.tif||TIFF image||8K||Figure S3. List of all the equations used in the model.|
|grl29763-sup-0005-txts01.txt||plain text document||10K||Text S1. Description of the model used to calculate the subsurface temperatures.|
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