Optical constants of Titan’s stratospheric aerosols in the 70–1500 cm−1 spectral range constrained by Cassini/CIRS observations
暂无分享,去创建一个
B. Bézard | C. Anderson | P. Rannou | R. Samuelson | S. Vinatier | R. Kok
[1] Jean-Jacques Correia,et al. Mid- and far-infrared absorption spectroscopy of Titan's aerosols analogues , 2012 .
[2] C. McKay,et al. Optical constants of Titan tholins at mid-infrared wavelengths (2.5–25 μm) and the possible chemical nature of Titan’s haze particles , 2012 .
[3] L. Brown,et al. High resolution investigation of the 7 μm region of the ethane spectrum , 2012 .
[4] B. Funke,et al. An unidentified emission in Titan's upper atmosphere , 2011 .
[5] C. Anderson,et al. Titan’s aerosol and stratospheric ice opacities between 18 and 500 μm: Vertical and spectral characteristics from Cassini CIRS , 2011 .
[6] Markus Kraft,et al. SURFACE CHEMISTRY AND PARTICLE SHAPE: PROCESSES FOR THE EVOLUTION OF AEROSOLS IN TITAN's ATMOSPHERE , 2011 .
[7] Conor A. Nixon,et al. Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission II: Aerosol extinction profiles in the 600–1420 cm−1 spectral range , 2010 .
[8] C. Griffith,et al. Titan's vertical aerosol structure at the Huygens landing site: Constraints on particle size, density, charge, and refractive index , 2010 .
[9] Sandrine Guerlet. Température et composition de la stratosphère de Saturne à partir des données Cassini/CIRS , 2010 .
[10] C. Sotin,et al. Titan haze distribution and optical properties retrieved from recent observations , 2010 .
[11] Conor A. Nixon,et al. Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles , 2010 .
[12] D. Young,et al. Heavy ions, temperatures and winds in Titan's ionosphere: Combined Cassini CAPS and INMS observations , 2009 .
[13] M. Tomasko,et al. Limits on the size of aerosols from measurements of linear polarization in Titan’s atmosphere , 2009 .
[14] J. Flaud,et al. Titan’s prolific propane: The Cassini CIRS perspective , 2009, 0909.1794.
[15] P. Drossart,et al. Titan solar occultation observed by Cassini/VIMS: Gas absorption and constraints on aerosol composition , 2009 .
[16] Paul F. McMillan,et al. New experimental constraints on the composition and structure of tholins , 2008 .
[17] A. Bellucci. Analyse d'occultations solaires et stellaires par Titan observées par l'instrument Cassini/VIMS , 2008 .
[18] F. Hourdin,et al. Diagnostics of Titan’s stratospheric dynamics using Cassini/CIRS data and the 2-dimensional IPSL circulation model , 2008 .
[19] R. Yelle,et al. Origin of oxygen species in Titan's atmosphere , 2008 .
[20] Roger V. Yelle,et al. Formation and distribution of benzene on Titan , 2008 .
[21] Mark T. Lemmon,et al. A model of Titan's aerosols based on measurements made inside the atmosphere , 2008 .
[22] Roger V. Yelle,et al. Ion chemistry and N-containing molecules in Titan's upper atmosphere , 2007 .
[23] David T. Young,et al. Discovery of heavy negative ions in Titan's ionosphere , 2007 .
[24] F. Flasar,et al. Characteristics of Titan's stratospheric aerosols and condensate clouds from Cassini CIRS far-infrared spectra , 2007 .
[25] J. Waite,et al. The Process of Tholin Formation in Titan's Upper Atmosphere , 2007, Science.
[26] B. Reynard,et al. Reflectance spectra and chemical structure of Titan's tholins: Application to the analysis of Cassini–Huygens observations , 2006 .
[27] C. McKay,et al. A coupled dynamics-microphysics model of Titan's atmosphere , 2004 .
[28] S. Atreya,et al. Current state of modeling the photochemistry of Titan's mutually dependent atmosphere and ionosphere , 2004 .
[29] 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 .
[30] Christopher P. McKay,et al. Analysis of the Time-Dependent Chemical Evolution of Titan Haze Tholin , 2002 .
[31] C. McKay,et al. A wind origin for Titan's haze structure , 2002, Nature.
[32] Frédéric Hourdin,et al. Seasonal Variations of Titan's Atmospheric Composition , 2001 .
[33] W. J. Lafferty,et al. First high resolution analysis of the absorption spectrum of propane in the 6.7 μm to 7.5 μm spectral region , 2001 .
[34] G. Socrates,et al. Infrared and Raman characteristic group frequencies : tables and charts , 2001 .
[35] R. Botet,et al. Mean-field approximation of Mie scattering by fractal aggregates of identical spheres. , 1997, Applied optics.
[36] R. Botet,et al. A new interpretation of scattered light measurements at Titan's limb , 1997 .
[37] E. Chassefière,et al. Formation and growth of photochemical aerosols in Titan's atmosphere , 1992 .
[38] D. Lide. Handbook of Chemistry and Physics , 1992 .
[39] D. Lin-Vien. The Handbook of Infrared and Raman Characteristic Frequencies of Organic Molecules , 1991 .
[40] A. Coustenis,et al. Titan's atmosphere from voyager infrared observations: III. Vertical distributions of hydrocarbons and nitriles near Titan's North Pole , 1991 .
[41] M. W. Williams,et al. Optical constants of organic tholins produced in a simulated Titanian atmosphere: From soft x-ray to microwave frequencies , 1984 .
[42] Z. Kam,et al. Absorption and Scattering of Light by Small Particles , 1998 .
[43] David Dolphin,et al. Tabulation of infrared spectral data , 1977 .
[44] R. Silverstein,et al. Spectrometric identification of organic compounds , 2013 .