dc.contributor.author |
Ivanov, A. B. |
en_US |
dc.contributor.author |
Muhleman, D. O. |
en_US |
dc.date.accessioned |
2004-09-22T22:24:01Z |
|
dc.date.available |
2004-09-22T22:24:01Z |
|
dc.date.issued |
2000-03-12 |
en_US |
dc.identifier.citation |
Lunar and Planetary Science Conference |
en_US |
dc.identifier.citation |
Houston, TX, USA |
en_US |
dc.identifier.clearanceno |
01-0177 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/12225 |
|
dc.description.abstract |
We present an algorithm to calculate the normal albedo of Mars at the MOLA wavelength using the MGS Thermal Emission Spectrometer (TES) 9 um opacity measurement [6]. |
en_US |
dc.format.extent |
271106 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
surface albedo reflected signal analysis MOLA Mars Orbiter Laser Altimeter |
en_US |
dc.title |
Reflected signal analysis and surface albedo in the Mars Orbiter Laser Altimeter (MOLA) |
en_US |