Physics
Scientist
Department of Geological Science, Brown University, Box 1846, Providence, RI 02912-1846, USA
NASA. Johnson Space Center, Houston, TX, US
Department of Geological Sciences, Brown University, Box 1846, Providence, RI 02912
Brown University
Brown University, Providence, Japan;
Department of Geological Sciences, Brown University, Box 1846, Providence, RI 02912-1846, USA
Brown University, Department of Geological Sciences, Providence, RI 02912, USA University, USA
Geological Institute, School of Science, University of Tokyo, Tokyo 113-0033, Japan
Brown Univ., Providence, RI.
Department of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
Department of Geological Sciences, Brown University, Providence, RI 02912, USA
NASA, Johnson Space Center, Houston, TX
National Aeronautics and Space Administration. Lyndon B. Johnson Space Center, Houston, TX.
Department of Geological Science, Brown University, Providence, RI 02912, USA
Brown University, Providence, RI, USA
Department of Geological Sciences, Brown University, Providence, Rhode Island, USA
Tokyo, University, Japan
Department of Geological Sciences, Brown University, Providence, Rhode Island 02912, USA
SN3, NASA Johnson Space Center, Houston, Texas
Department of Geological Sciences, Brown University, Box 1846, Providence, Rhode Island 02912, USA
Department of Geological Sciences, Brown University, Rhode Island 02912, USA
NASA-ARC, Mail Stop 239-4, Moffett Field, California 94035, USA of Geological Sciences, Brown University, Providence RI 02912, USA
3-µm Spectroscopic Obersvations of Asteroid 21 Lutetia Using Akari Satellite
A Method of Converting Reflectance Spectra into Absorption Coefficient Spectra of Mineral Mixtures for Application to Asteroidal Surface Mineralogy
A method to determine silicate abundances from reflectance spectra with applications to Asteroid 29 amphitrite associating it with primitive achondrite meteorites
A new Antarctic meteorite with chromite, orthopyroxene and metal with reference to a formation model of S asteroids
A New Modified Gaussian Model (MGM) Using a Bayesian Estimation Approach: Toward Automated Analysis of Planetary Spectra
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