Computer Science
Scientist
Hawaii University
Department of Earth and Space Science, University of Washington, Seattle, WA 98195, USA / SOEST, University of Hawaii
Hawaii Inst. of Geophys. & Planet., University of Hawaii
Planetary Science Institute
PSI
University of Washington, Department of Earth and Space Science Box 351310, Seattle, WA 98195-1310
Planetary Science Institute, 22 Fiddler's Rd., Winthrop WA 98862-0667
Planetary Sci. Inst.
University of Washington, Department of Earth and Space Science Box 351310, Seattle, WA 98195-1310, USA
Planetary Science Instutute
The Planetary Science Institute
University of Washington
Planetary Science Institute, 22 Fiddler's Rd., Winthrop, WA 98862-0667, USA
HIGP / SOEST University of Hawaii
University of Washington, Seattle, WA, USA
University of Washington, Department of Eaarth and Space Sciences, Seattle, WA 98195 of Hawaii, HIGP / SOEST 2525 Correa Rd., Honololu, HI 96822 Inst. Gephys. Planet., SOEST University of Hawaii, 2525 Correa Rd., Honolulu, HI 96822, USA Fight Center, 22 Fiddler's Rd., Winthrop, WA 98862-0667, USA
University of Washington, Department of Earth and Space Science, Seattle, WA 98195, USA of Washington, Earth and Space Science, Seattle, WA 98195
Planetary Science Institute, 225 South Lake Avenue, Pasadena, CA 91101.
Department of Earth and Space Sciences, University of Washington, Box 351310, Seattle, WA 98195-1310, USA
Planetary Science Institute, 225 S. Lake Ave. Suite 300, Pasadena, Ca 91101 of Earth and Space Sciences, Johnson Annex A, Box 351310, University of Washington, Seattle WA 98195, USA
Earth & Space Sciences, University of Washington, Seattle, WA, USA and Space Sciences, University of Washing
A close look at Saturn's rings with Cassini VIMS
A first analysis of Callisto using Galileo NIMS and SSI measurements
A Method of Measuring Surface Ice Abundance: Application to Ganymede
A microphysically-based approach to modeling emissivity and albedo of the martian seasonal caps
Albedo models for the residual south polar cap on Mars: Implications for the stability of the cap under near-perihelion global dust storm conditions
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