94 results on '"Cruikshank, Dale P."'
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2. Analysis of Charon’s spectrum at 2.21-μm from New Horizons/LEISA and Earth-based observations
3. Stress-activated electric currents in icy planetary bodies: H2O2-doped H2O ices
4. Cryovolcanic flooding in Viking Terra on Pluto
5. Probing the regoliths of the classical Uranian satellites: Are their surfaces mantled by a layer of tiny H2O ice grains?
6. The distribution of H2O, CH3OH, and hydrocarbon-ices on Pluto: Analysis of New Horizons spectral images
7. Recent cryovolcanism in Virgil Fossae on Pluto
8. Erratum to ‘Isotopic Ratios of Saturn's Rings and Satellites: Implications for the Origin of Water and Phoebe’ [ICARUS 321 (2019) 791–802]
9. Isotopic ratios of Saturn's rings and satellites: Implications for the origin of water and Phoebe
10. Composition of Pluto’s small satellites: Analysis of New Horizons spectral images
11. Asteroid (16) Psyche: Evidence for a silicate regolith from spitzer space telescope spectroscopy
12. Bladed Terrain on Pluto: Possible origins and evolution
13. Cassini's geological and compositional view of Tethys
14. Saturn’s icy satellites investigated by Cassini-VIMS. IV. Daytime temperature maps
15. The Veritas and Themis asteroid families: 5–14 µ m spectra with the Spitzer Space Telescope
16. Impact craters: An ice study on Rhea
17. Aromatic and aliphatic organic materials on Iapetus: Analysis of Cassini VIMS data
18. The temperature and width of an active fissure on Enceladus measured with Cassini VIMS during the 14 April 2012 South Pole flyover
19. A compositional interpretation of trans-neptunian objects taxonomies
20. Infrared spectroscopic characterization of the low-albedo materials on Iapetus
21. Compositional analysis of Hyperion with the Cassini Visual and Infrared Mapping Spectrometer
22. The surface composition of Iapetus: Mapping results from Cassini VIMS
23. Optical constants of Titan tholins at mid-infrared wavelengths (2.5–25μm) and the possible chemical nature of Titan’s haze particles
24. The Saturnian satellite Rhea as seen by Cassini VIMS
25. Iapetus surface variability revealed from statistical clustering of a VIMS mosaic: The distribution of CO2
26. Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
27. A search for ethane on Pluto and Triton
28. Carbon dioxide on the satellites of Saturn: Results from the Cassini VIMS investigation and revisions to the VIMS wavelength scale
29. Dione’s spectral and geological properties
30. Eclipse reappearances of Io: Time-resolved spectroscopy (1.9–4.2μm)
31. VIMS spectral mapping observations of Titan during the Cassini prime mission
32. Fluvial erosion and post-erosional processes on Titan
33. Hydrocarbons on Saturn's satellites Iapetus and Phoebe
34. Compositional mapping of Saturn's satellite Dione with Cassini VIMS and implications of dark material in the Saturn system
35. A close look at Saturn's rings with Cassini VIMS
36. Correlations between Cassini VIMS spectra and RADAR SAR images: Implications for Titan's surface composition and the character of the Huygens Probe Landing Site
37. Carbon dioxide on planetary bodies: Theoretical and experimental studies of molecular complexes
38. Tholins as coloring agents on outer Solar System bodies
39. Solar system observations with Spitzer Space Telescope: Preliminary results
40. Laboratory experiments of Titan tholin formed in cold plasma at various pressures: implications for nitrogen-containing polycyclic aromatic compounds in Titan haze
41. Quantitative modeling of the spectral reflectance of Kuiper Belt objects and Centaurs
42. The 1.95–2.50 μm Spectrum of J6 Himalia
43. Detection of Sub-Micron Radiation from the Surface of Venus by Cassini/VIMS
44. Composition, Physical State, and Distribution of Ices at the Surface of Triton
45. Water Ice on Nereid
46. The Detection of Water Ice in Comet Hale-Bopp
47. Near-Infrared Spectral Geometric Albedos of Charon and Pluto: Constraints on Charon's Surface Composition
48. Temperature of Nitrogen Ice on Pluto and Its Implications for Flux Measurements
49. Infrared Spectroscopy of Triton and Pluto Ice Analogs: The Case for Saturated Hydrocarbons
50. Spectroscopy of Mars from 2.04 to 2.44μm during the 1993 Opposition: Absolute Calibration and Atmospheric vs Mineralogic Origin of Narrow Absorption Features
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