Numerical modeling of lava-regolith heat transfer on the Moon and implications for the preservation of implanted volatiles
Article first published online: 8 MAR 2013
©2012. American Geophysical Union. All Rights Reserved.
Journal of Geophysical Research: Planets
Volume 118, Issue 3, pages 382–397, March 2013
How to Cite
2013), Numerical modeling of lava-regolith heat transfer on the Moon and implications for the preservation of implanted volatiles, J. Geophys. Res. Planets, 118, 382–397, , , and (
- Issue published online: 25 APR 2013
- Article first published online: 8 MAR 2013
- Manuscript Accepted: 12 DEC 2012
- Manuscript Revised: 21 NOV 2012
- Manuscript Received: 18 MAY 2012
All Supporting Information may be found in the online version of this article.
|2012JE004131fs01.eps||PS document||75190K||Auxillary Figure. Temperature profiles through lava and regolith at (a) 1 day, (b) 10 days, (c) 20 days, and (d) 50 days after emplacement of 1 m thick lava flow, with all thermophysical parameters held constant. Orange line represents an ambient temperature (T∞) of 4 K. Tan line represents effective ambient temperature of 250 K. Initial lava and regolith temperatures are 1500 K and 200 K, respectively. Vertical dashed lines indicate temperatures at which specific particles will begin to volatilize (Table 1).|
|2012JE004131readme.txt||plain text document||1K||Supporting Information|
Please note: Wiley Blackwell is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.