Wellesley College, Department of Astronomy
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- Cassini Radio Occultation Results for Saturn's Rings
- Density Waves in Saturn's Rings from Cassini Radio Occultations
- Low-latitude Temperatures, Pressures, and Winds on Saturn from Cassini Radio Occultations
- Scattered Signal Observations During Cassini Radio Occultations by Saturn's Rings
- Vertically Propagating Waves in the Upper Atmosphere of Saturn From Cassini Radio Occultations
- Cassini Radio Occultation by Enceladus Plume
- Evidence for Likely Liquid Hydrocarbons on Titan's Surface from Cassini Radio Science Bistatic Scattering Observations
- Statistical Modeling and Characterization of Microstructure in Saturn's Rings
- Thermal Structure of Titan's Atmosphere from Cassini Radio Occultations and Thermal- Infrared Spectra
- Characterization of Enigmatic Saturn's Ring B by Cassini Radio Occultations
- Results from the 2007 Radio Occultations of Cassini by Saturn
- The Meridional and Vertical Structure of Titan's Atmosphere from Cassini Radio Occultations
- The electron density structure of the Titan ionosphere
- Dielectric Constant of Titan's South Polar Region from Cassini Radio Science Bistatic Scattering Observations
- Saturn's Titan and Maxwell Ringlets from Cassini RSS Observations
- Planetary Rings: Circular and Non-circular
- Six Centuries Old Spiral of Vertical Corrugations in Saturn's C-Ring
- Paleotopography of Husband Hill and the West Spur of the Columbia Hills, Gusev Crater, Mars
- Reconstructed Paleo-topography of the Columbia Hills, Mars
- Seasonal Variations in Pluto's Atmospheric Tides
- Exploring Regolith Depth and Cycling on Mars
- 100-meter Resolution Characterization of Structure in Saturn's Rings with Cassini Radio Occultations
- Particle sizes in Saturn's rings from Cassini UVIS, VIMS, and RSS Occultations.
- Spatio-Temporal Structure of Titan's Atmosphere from Radio Occultations over the Cassini Mission
- The Shape of Saturn's A Ring Edge from Cassini VIMS, UVIS, and RSS Occultations
- The Shape of Saturn's B Ring Edge from Voyager, Earth-based, and Cassini VIMS, UVIS, and RSS Occultations
- Measuring the Stratospheric Temperature of Uranus Using Archival Stellar Occultations