Surface roughness of Mars

Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2004. === Includes bibliographical references (p. 35-36). === In this thesis, I created an algorithm to compensate for the saturation of data collected by the Mars Orbiter Laser Altimeter (MOLA). Saturation of the energy measure...

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Main Author: Mamo, Andrew Benedict, 1982-
Other Authors: Maria T. Zuber.
Format: Others
Language:English
Published: Massachusetts Institute of Technology 2006
Subjects:
Online Access:http://hdl.handle.net/1721.1/32744
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spelling ndltd-MIT-oai-dspace.mit.edu-1721.1-327442019-05-02T16:11:22Z Surface roughness of Mars Mamo, Andrew Benedict, 1982- Maria T. Zuber. Massachusetts Institute of Technology. Dept. of Physics. Massachusetts Institute of Technology. Dept. of Physics. Physics. Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2004. Includes bibliographical references (p. 35-36). In this thesis, I created an algorithm to compensate for the saturation of data collected by the Mars Orbiter Laser Altimeter (MOLA). Saturation of the energy measurements had made it impossible to measure surface roughness at 100 m length scales. By calculating the returned energy, the problem of saturation can be avoided. This algorithm was applied to MOLA data across the Martian surface to create an estimate of surface roughness across the planet. The method calculates pulse spreading from returned pulse energy using the link equation. The accuracy of the method is limited by the accuracy of albedo measurements. This analysis improved the estimation of surface roughness on Mars. Further improvements could be gained by correcting for the opacity of atmospheric dust as a cause of pulse spreading. by Andrew Benedict Mamo. S.B. 2006-05-15T20:26:55Z 2006-05-15T20:26:55Z 2004 2004 Thesis http://hdl.handle.net/1721.1/32744 56733837 eng M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 36 p. 1272804 bytes 1272262 bytes application/pdf application/pdf application/pdf zma---- Massachusetts Institute of Technology
collection NDLTD
language English
format Others
sources NDLTD
topic Physics.
spellingShingle Physics.
Mamo, Andrew Benedict, 1982-
Surface roughness of Mars
description Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2004. === Includes bibliographical references (p. 35-36). === In this thesis, I created an algorithm to compensate for the saturation of data collected by the Mars Orbiter Laser Altimeter (MOLA). Saturation of the energy measurements had made it impossible to measure surface roughness at 100 m length scales. By calculating the returned energy, the problem of saturation can be avoided. This algorithm was applied to MOLA data across the Martian surface to create an estimate of surface roughness across the planet. The method calculates pulse spreading from returned pulse energy using the link equation. The accuracy of the method is limited by the accuracy of albedo measurements. This analysis improved the estimation of surface roughness on Mars. Further improvements could be gained by correcting for the opacity of atmospheric dust as a cause of pulse spreading. === by Andrew Benedict Mamo. === S.B.
author2 Maria T. Zuber.
author_facet Maria T. Zuber.
Mamo, Andrew Benedict, 1982-
author Mamo, Andrew Benedict, 1982-
author_sort Mamo, Andrew Benedict, 1982-
title Surface roughness of Mars
title_short Surface roughness of Mars
title_full Surface roughness of Mars
title_fullStr Surface roughness of Mars
title_full_unstemmed Surface roughness of Mars
title_sort surface roughness of mars
publisher Massachusetts Institute of Technology
publishDate 2006
url http://hdl.handle.net/1721.1/32744
work_keys_str_mv AT mamoandrewbenedict1982 surfaceroughnessofmars
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