An upper limit for ice in Shackleton crater as revealed by LRO Mini-RF orbital radar
Version of Record online: 28 JUL 2012
©2012. American Geophysical Union. All Rights Reserved.
Geophysical Research Letters
Volume 39, Issue 14, 28 July 2012
How to Cite
2012), An upper limit for ice in Shackleton crater as revealed by LRO Mini-RF orbital radar, Geophys. Res. Lett., 39, L14201, doi:10.1029/2012GL052119., et al. (
- Issue online: 28 JUL 2012
- Version of Record online: 28 JUL 2012
- Manuscript Accepted: 16 JUN 2012
- Manuscript Revised: 15 JUN 2012
- Manuscript Received: 23 APR 2012
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|grl29310-sup-0001-readme.txt||plain text document||2K||readme.txt|
|grl29310-sup-0002-txts01.pdf||PDF document||20K||Text S1. Description of the ice-regolith mixing model used to produce the synthetic radar images given inFigures 2a–2c.|
|grl29310-sup-0003-fs01.jpg||JPEG image||277K||Figure S1. Modeled circular polarization ratio values as a function of incidence angle for a mixture of lunar regolith and water ice.|
|grl29310-sup-0004-fs02.jpg||JPEG image||442K||Figure S2. Topographically-corrected Mini-RF CPR data of Shackleton fromFigure 2a.|
|grl29310-sup-0005-fs03.jpg||JPEG image||419K||Figure S3. Topographically-corrected Mini-RF SC and OC data of Shackleton fromFigure 2a.|
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