The geology of Hotei Regio, Titan: Correlation of Cassini VIMS and RADAR

[1]  S. Hensley,et al.  Titan's Rotation Reveals an Internal Ocean and Changing Zonal Winds , 2008, Science.

[2]  Trent M. Hare,et al.  Topography and geomorphology of the Huygens landing site on Titan , 2007 .

[3]  A. Aikin,et al.  C4H2, HC3N and C2N2 in Titan's atmosphere , 1981, Nature.

[4]  C. Sotin,et al.  Titan's surface: Search for spectral diversity and composition using the Cassini VIMS investigation , 2008 .

[5]  J. Lunine,et al.  Clathrate and Ammonia Hydrates at High Pressure: Application to the Origin of Methane on Titan , 1987 .

[6]  Bonnie J. Buratti,et al.  Composition of Titan's surface from Cassini VIMS , 2006 .

[7]  D. Hunten,et al.  The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probe , 2005, Nature.

[8]  Gabriel Tobie,et al.  Titan's internal structure inferred from a coupled thermal-orbital model , 2005 .

[9]  C. Sotin,et al.  Spectroscopy, morphometry, and photoclinometry of Titan's dunefields from Cassini/VIMS , 2008 .

[10]  P. Grindrod,et al.  Modelling of possible mud volcanism on Titan , 2006 .

[11]  C. McKay,et al.  Complex refractive indices of tholins produced from various initial gas mixtures and formation pressures: Implications for Titan, the early Earth, and the outer solar system bodies , 2005 .

[12]  Christopher P. McKay,et al.  Physical properties of the organic aerosols and clouds on Titan , 2001 .

[13]  Christopher P. McKay,et al.  Formation of methane in comet impacts: implications for Earth, Mars, and Titan , 2004 .

[14]  T. Watters,et al.  Coronae on Venus and Mars: Implications for similar structures on Earth , 1995 .

[15]  R. H. Brown,et al.  The identification of liquid ethane in Titan’s Ontario Lacus , 2008, Nature.

[16]  R. Lorenz,et al.  Liquids and solids on the surface of Titan , 1994 .

[17]  Rosaly M. C. Lopes,et al.  Resurfacing of Titan by ammonia-water cryomagma , 2005 .

[18]  P. Drossart,et al.  Evidence for a Polar Ethane Cloud on Titan , 2006, Science.

[19]  J. Waite,et al.  The source of heavy organics and aerosols in Titan's atmosphere , 2008, Proceedings of the International Astronomical Union.

[20]  C. Sotin,et al.  Episodic outgassing as the origin of atmospheric methane on Titan , 2005, Nature.

[21]  Rosaly M. C. Lopes,et al.  The Sand Seas of Titan: Cassini RADAR Observations of Longitudinal Dunes , 2006, Science.

[22]  R. Kirk,et al.  Rain, winds and haze during the Huygens probe's descent to Titan's surface , 2005, Nature.

[23]  T. Tokano,et al.  Wind‐induced seasonal angular momentum exchange at Titan's surface and its influence on Titan's length‐of‐day , 2005 .

[24]  R. Clark,et al.  Search for volatiles on icy satellites: I. Europa , 1988 .

[25]  Olivier Grasset,et al.  The Cooling Rate of a Liquid Shell in Titan's Interior , 1996 .

[26]  Christopher P. McKay,et al.  Laboratory experiments of Titan tholin formed in cold plasma at various pressures: implications for nitrogen-containing polycyclic aromatic compounds in Titan haze , 2004 .

[27]  G. Orton,et al.  The composition of Titan's stratosphere from Cassini/CIRS mid-infrared spectra , 2007 .

[28]  Rosaly M. C. Lopes,et al.  Three-Dimensional Views of Titan's Diverse Surface Features from Cassini RADAR Stereogrammetry , 2009 .

[29]  Jeffrey S. Kargel,et al.  Rheological properties of ammonia-water liquids and crystal-liquid slurries - Planetological applications , 1991 .

[30]  Randolph L. Kirk,et al.  Correlations between Cassini VIMS spectra and RADAR SAR images: Implications for Titan's surface composition and the character of the Huygens Probe Landing Site , 2007 .

[31]  Rosaly M. C. Lopes,et al.  Mountains on Titan observed by Cassini Radar , 2006 .

[32]  A. Mckellar.  The spectrum of gaseous methane at 77 K in the 1.1 – 2.6 μm region: a benchmark for planetary astronomy , 1989 .

[33]  D. Buczkowski.  Kinematic analysis of radial structures around Irnini Mons, Venus , 2006 .

[34]  F. Paganelli,et al.  Cassini RADAR images at Hotei Arcus and western Xanadu, Titan: Evidence for geologically recent cryovolcanic activity , 2009 .

[35]  Roberto Orosei,et al.  Cryovolcanic features on Titan's surface as revealed by the Cassini Titan Radar Mapper , 2007 .

[36]  Paul E. Lewis,et al.  MODTRAN5: 2006 update , 2006, SPIE Defense + Commercial Sensing.

[37]  W. Chadwick,et al.  The pattern of circumferential and radial eruptive fissures on the volcanoes of Fernandina and Isabela islands, Galapagos , 1991 .

[38]  Bonnie J. Buratti,et al.  Global-scale surface spectral variations on Titan seen from Cassini/VIMS , 2007 .

[39]  R. H. Brown,et al.  The Cassini Visual And Infrared Mapping Spectrometer (Vims) Investigation , 2004 .

[40]  B. Hapke,et al.  Saturn's Titan: Surface change, ammonia, and implications for atmospheric and tectonic activity , 2009 .

[41]  John J. Remedios,et al.  Improved near-infrared methane band models and k-distribution parameters from 2000 to 9500 cm(-1) and implications for interpretation of outer planet spectra , 2006 .

[42]  JOHN S. Lewis.  Physics And Chemistry Of The Solar System , 1995 .

[43]  C. Sotin,et al.  Detection and mapping of hydrocarbon deposits on Titan , 2010 .

[44]  C. Sotin,et al.  Cassini observations of flow‐like features in western Tui Regio, Titan , 2006 .

[45]  C. Sotin,et al.  A 5-Micron-Bright Spot on Titan: Evidence for Surface Diversity , 2005, Science.

[46]  Mark T. Lemmon,et al.  Titan's Surface, Revealed by HST Imaging , 1996 .

[47]  A. Showman,et al.  Thermal convection in ice-I shells of Titan and Enceladus , 2006 .

[48]  Rosaly M. C. Lopes,et al.  Dunes on Titan observed by Cassini Radar , 2008 .