Saturn's icy satellites investigated by Cassini-VIMS. I. Full-disk properties: 350-5100 nm reflectance spectra and phase curves
暂无分享,去创建一个
C. Sotin | P. Drossart | R. Clark | M. Showalter | R. Jaumann | B. Buratti | A. Coradini | T. McCord | R. Nelson | K. Baines | D. Matson | Y. Langevin | J. Bibring | M. Combes | V. Formisano | G. Filacchione | F. Capaccioni | P. Cerroni | Robert H. Brown | G. Bellucci | D. Cruikshank | B. Sicardy | E. D'Aversa | V. Mennella | F. Tosi | P. Nicholson | V. Formisano | G. Hansen | K. Hibbitts | S. Newman | E. D’Aversa | E. D’aversa | Robert H. Brown | R. Clark
[1] S. Sandford,et al. Optical constants of amorphous and crystalline H2O-ice in the near infrared from 1.1 to 2.6 μm , 2008 .
[2] E. Grün,et al. The E ring in the vicinity of Enceladus - I. Spatial distribution and properties of the ring particles , 2008 .
[3] J. Bauer,et al. Photometric and spectral analysis of the distribution of crystalline and amorphous ices on Enceladus as seen by Cassini , 2008 .
[4] P. Thomas,et al. Saturn's Small Inner Satellites: Clues to Their Origins , 2007, Science.
[5] P. Thomas,et al. The Equatorial Ridges of Pan and Atlas: Terminal Accretionary Ornaments? , 2007, Science.
[6] R. Clark,et al. Compositional mapping of Saturn's satellite Dione with Cassini VIMS and implications of dark material in the Saturn system , 2007 .
[7] Robert H. Brown,et al. A Possible Trace Carbon Dioxide Polar Cap on Iapetus , 2007 .
[8] R. H. Brown,et al. Surface composition of Hyperion , 2007, Nature.
[9] D. Cruikshank,et al. Carbon dioxide on planetary bodies: Theoretical and experimental studies of molecular complexes , 2007 .
[10] C. Sotin,et al. Distribution of icy particles across Enceladus' surface as derived from Cassini-VIMS measurements , 2007 .
[11] F. Scholten,et al. High-resolution CASSINI-VIMS mosaics of Titan and the icy Saturnian satellites , 2006 .
[12] Robert H. Brown,et al. Ion irradiation of crystalline H2O–ice: Effect on the 1.65-μm band , 2006 .
[13] E. Bergin,et al. Synthesis of CO and CO2 Molecules by UV Irradiation of Water Ice-covered Hydrogenated Carbon Grains , 2006 .
[14] M. Skrutskie,et al. Near-infrared spectra of the leading and trailing hemispheres of Enceladus , 2006 .
[15] J. Kargel,et al. Enceladus: Cosmic Gymnast, Volatile Miniworld , 2006, Science.
[16] R. Jaumann,et al. Composition and Physical Properties of Enceladus' Surface , 2006, Science.
[17] C. Sotin,et al. VIS-NIR spectral properties of Saturn's minory icy moons , 2006 .
[18] C. Sotin,et al. Iapetus, Phoebe and Hyperion: are they related? , 2006 .
[19] Jonathan I. Lunine,et al. Saturn's moon Phoebe as a captured body from the outer Solar System , 2005, Nature.
[20] Ralf Jaumann,et al. Compositional maps of Saturn's moon Phoebe from imaging spectroscopy , 2005, Nature.
[21] T. Owen,et al. A spectroscopic study of the surfaces of Saturn's large satellites: H 2 O ice, tholins, and minor constituents , 2005 .
[22] J. B. Dalton,et al. Near-infrared (0.8-4.0 μm) spectroscopy of Mimas, Enceladus, Tethys, and Rhea , 2005 .
[23] R. H. Brown,et al. Cassini Visual and Infrared Mapping Spectrometer Observations of Iapetus: Detection of CO2 , 2005 .
[24] D. Strobel,et al. Atmospheres and Plasma Interactions at Saturn’s Largest Inner Icy Satellites , 2005 .
[25] M. Showalter,et al. Keck near-infrared observations of Saturn's E and G rings during Earth's ring plane crossing in August 1995 , 2004 .
[26] R. H. Brown,et al. The Cassini Visual And Infrared Mapping Spectrometer (Vims) Investigation , 2004 .
[27] C. Sotin,et al. Cassini VIMS observations of the Galilean satellites including the VIMS calibration procedure , 2004 .
[28] C. Barbieri,et al. Water ice on the surface of the large TNO 2004 DW , 2004 .
[29] A. Coradini,et al. CASSINI/VIMS-V at Jupiter: Radiometric calibration test and data results , 2004 .
[30] T. Roush,et al. Compositions of Saturn's rings A, B, and C from high resolution near-infrared spectroscopic observations , 2003 .
[31] D. Cruikshank,et al. Spectral Models of Kuiper Belt Objects and Centaurs , 2003 .
[32] M. Barucci,et al. Ion Irradiation of Asphaltite: Optical Effects and Implications for Trans-Neptunian Objects and Centaurs , 2003 .
[33] T. McCord,et al. Amorphous and crystalline ice on the Galilean satellites: A balance between thermal and radiolytic processes , 2003 .
[34] F. Poulet,et al. The Composition of Saturn's Rings , 2002 .
[35] B. Buratti,et al. High-Resolution 0.33–0.92 μm Spectra of Iapetus, Hyperion, Phoebe, Rhea, Dione, and D-Type Asteroids: How Are They Related? , 2002 .
[36] J. Richardson,et al. Satellite sputtering in Saturn's magnetosphere , 2001 .
[37] K. Baines,et al. The Saturnian Satellites in the Near-Infrared: Absolute Photometry at Ring Plane Crossing , 2000 .
[38] T. Owen,et al. Water Ice on Triton , 2000 .
[39] M. Gaffey,et al. Are Hyperion and Phoebe Linked to Iapetus , 2000 .
[40] Marc William Buie,et al. Near-Infrared Spectra of Icy Outer Solar System Surfaces: Remote Determination of H2O Ice Temperatures , 1999 .
[41] Gabriele Arnold,et al. OPPOSITION EFFECT FROM CLEMENTINE DATA AND MECHANISMS OF BACKSCATTER , 1999 .
[42] T. Roush,et al. Detection of Water Ice on Saturn's Satellite Phoebe , 1999 .
[43] P. Ehrenfreund,et al. The infrared band strengths of CH_3OH, NH_3 and CH_4 in laboratory simulations of astrophysical ice mixtures , 1999 .
[44] I. Shapiro,et al. Mainbelt Asteroids: Results of Arecibo and Goldstone Radar Observations of 37 Objects during 1980-1995 , 1998 .
[45] Bernard Schmitt,et al. The temperature‐dependent near‐infrared absorption spectrum of hexagonal H2O ice , 1998 .
[46] A. Coradini,et al. Imaging spectroscopy of Saturn and its satellites : vims-v onboard Cassini , 1998 .
[47] William D. Smythe,et al. The Opposition Effect of the Moon: Coherent BackscatterandShadow Hiding , 1998 .
[48] James Charles Granahan,et al. Non‐water‐ice constituents in the surface material of the icy Galilean satellites from the Galileo near‐infrared mapping spectrometer investigation , 1998 .
[49] G. Hansen. The infrared absorption spectrum of carbon dioxide ice from 1.8 to 333 μm , 1997 .
[50] R. E. Johnson,et al. Detection of ozone on Saturn's satellites Rhea and Dione , 1997, Nature.
[51] Stephen M. Larson,et al. Unraveling the Zebra: Clues to the Iapetus Dark Material Composition , 1996 .
[52] Michele Dami,et al. The Visual and Infrared Mapping Spectrometer for Cassini , 1996, Optics & Photonics.
[53] C. Sagan,et al. SPECTROPHOTOMETRY AND ORGANIC MATTER ON IAPETUS. 2 : MODELS OF INTERHEMISPHERIC ASYMMETRY , 1996 .
[54] T. Owen,et al. The Surface Compositions of Triton, Pluto, and Charon , 1995 .
[55] B. Buratti. The Dark Side of Iapetus: Additional Evidence for an Exogenous Origin , 1995 .
[56] David P. Hamilton,et al. Origin of Saturn's E Ring: Self-Sustained, Naturally , 1994, Science.
[57] B. Hapke. Theory of reflectance and emittance spectroscopy , 1993 .
[58] R. Matthews. The Darkening of Iapetus and the Ongin of Hyperion , 1992 .
[59] W. Hartmann,et al. Solid CN bearing material on outer solar system bodies , 1991 .
[60] F. Spinella,et al. The 3.1 mu.m feature in ion-irradiated water ice. , 1991 .
[61] B. Buratti,et al. Albedo and color maps of the Saturnian satellites , 1990 .
[62] S. Sandford,et al. The physical and infrared spectral properties of CO2 in astrophysical ice analogs. , 1990, The Astrophysical journal.
[63] S. Warren. Optical constants of carbon dioxide ice. , 1986, Applied optics.
[64] G. Strazzulla. Organic material from Phoebe to Iapetus , 1986 .
[65] R. Clark,et al. Spectral properties of ice‐particulate mixtures and implications for remote sensing: 1. Intimate mixtures , 1984 .
[66] B. Hapke. Bidirectional reflectance spectroscopy , 1984 .
[67] R. Clark,et al. Saturn's satellites: Nuar-infrared spectrophotometry (0.6–2.5 μm) of the leading and trailing sides and compositional implications , 1984 .
[68] J. Veverka,et al. Voyager photometry of Rhea, Dione, Tethys, Enceladus and Mimas , 1984 .
[69] J. Lissauer,et al. Resonances in Saturn's rings , 1982 .
[70] B. Hapke. Bidirectional reflectance spectroscopy: 1. Theory , 1981 .
[71] Roger N. Clark,et al. Water frost and ice - The near-infrared spectral reflectance 0.65-2.5 microns. [observed on natural satellites and other solar system objects , 1981 .
[72] U. Fink,et al. Temperature dependence of the water-ice spectrum between 1 and 4 microns - Application to Europa, Ganymede and Saturn's rings , 1975 .
[73] O. Franz,et al. Photometry of Dione, Tethys, and Enceladus on the UBV system , 1975 .
[74] T. McCord,et al. Saturn and its satellites - Narrow-band spectrophotometry, 0.3-1.1 micron , 1971 .
[75] R. Clark,et al. Ring Particle Composition and Size Distribution , 2009 .
[76] Angioletta Coradini,et al. Identification of spectral units on Phoebe , 2008 .
[77] P. Drossart,et al. A close look at Saturn's rings with Cassini VIMS , 2008 .
[78] R. French,et al. The opposition surge of Enceladus: HST observations 338–1022 nm , 2005 .
[79] Dale P. Cruikshank,et al. Ices on the Satellites of Jupiter, Saturn, and Uranus , 1995 .
[80] R. Clark,et al. Surface composition of natural satellites. , 1986 .
[81] Bradford A. Smith,et al. Satellites of Saturn - Geological perspective , 1984 .
[82] Robert N. Colwell,et al. Manual of remote sensing , 1983 .