Analysis of gaseous ammonia (NH3) absorption in the visible spectrum of Jupiter - Update
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Jonathan Tennyson | Sergey N. Yurchenko | Ryan Garland | Neil Bowles | J. Tennyson | S. Calcutt | N. Bowles | P. Irwin | A. Braude | Patrick G. J. Irwin | S. Yurchenko | Phillip A. Coles | Simon Calcutt | R. Garland | Ashwin S. Braude
[1] G. Orton,et al. Colour and tropospheric cloud structure of Jupiter from MUSE/VLT: Retrieving a universal chromophore , 2019, Icarus.
[2] P. Irwin,et al. Effectively Calculating Gaseous Absorption in Radiative Transfer Models of Exoplanetary and Brown Dwarf Atmospheres , 2019, 1903.03997.
[3] J. Tennyson,et al. Improved potential energy surface and spectral assignments for ammonia in the near-infrared region , 2018, Journal of Quantitative Spectroscopy and Radiative Transfer.
[4] P. Bernath,et al. Analysis of the red and green optical absorption spectrum of gas phase ammonia , 2018 .
[5] K. Baines,et al. A possibly universal red chromophore for modeling color variations on Jupiter , 2017, 1706.02779.
[6] Ahmed F. Al-Refaie,et al. The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres , 2016, 1603.05890.
[7] G. Orton,et al. Reanalysis of Uranus' cloud scattering properties from IRTF/SpeX observations using a self-consistent scattering cloud retrieval scheme , 2015, 1601.02814.
[8] J. Tennyson,et al. Spectrum of hot methane in astronomical objects using a comprehensive computed line list , 2014, Proceedings of the National Academy of Sciences.
[9] J. Manners,et al. Accuracy tests of radiation schemes used in hot Jupiter global circulation models , 2014, 1402.0814.
[10] Jonathan Tennyson,et al. ExoMol line lists - III. An improved hot rotation-vibration line list for HCN and HNC , 2013, 1311.1328.
[11] K. Baines,et al. Chromophores from photolyzed ammonia reacting with acetylene: Application to Jupiter's Great Red Spot , 2012 .
[12] J. Tennyson,et al. ExoMol: molecular line lists for exoplanet and other atmospheres , 2012, 1204.0124.
[13] J. Tennyson,et al. Towards efficient refinement of molecular potential energy surfaces: Ammonia as a case study , 2011 .
[14] J. Tennyson,et al. A variationally computed line list for hot NH3 , 2010, 1011.1569.
[15] M. Loupias,et al. The MUSE second-generation VLT instrument , 2010, Astronomical Telescopes + Instrumentation.
[16] Kelly Chance,et al. An improved high-resolution solar reference spectrum for earth's atmosphere measurements in the ultraviolet, visible, and near infrared , 2010 .
[17] M. Tomasko,et al. Methane absorption coefficients for the jovian planets from laboratory, Huygens, and HST data , 2010 .
[18] S. Calcutt,et al. Band parameters for self-broadened ammonia gas in the range 0.74 to 5.24 μm to support measurements of the atmosphere of the planet Jupiter , 2008 .
[19] S. Calcutt,et al. The NEMESIS planetary atmosphere radiative transfer and retrieval tool , 2008 .
[20] A. Burrows,et al. Atomic and Molecular Opacities for Brown Dwarf and Giant Planet Atmospheres , 2006, astro-ph/0607211.
[21] K. Banse,et al. Data reduction pipelines for the Very Large Telescope , 2006, SPIE Astronomical Telescopes + Instrumentation.
[22] Gang Li,et al. The HITRAN 2008 molecular spectroscopic database , 2005 .
[23] Steve Matousek,et al. The Juno New Frontiers mission , 2005 .
[24] T. Fouchet,et al. Retrievals of Jovian tropospheric phosphine from CassiniKIRS , 2004 .
[25] J. Orphal,et al. Temperature dependence of pressure broadening of NH3 perturbed by H2 and N2 , 2004 .
[26] Keeyoon Sung,et al. Measurements of line intensities and half-widths in the 10-μm bands of 14NH3 , 2004 .
[27] G. Thuillier,et al. The Solar Spectral Irradiance from 200 to 2400 nm as Measured by the SOLSPEC Spectrometer from the Atlas and Eureca Missions , 2003 .
[28] M. D. Rosa,et al. New results for the temperature dependence of self-broadening and shift in the v2 ammonia band , 2000 .
[29] A. Borysow,et al. Semi-empirical Model of Collision-Induced Absorption Spectra of H2–H2 Complexes in the Second Overtone Band of Hydrogen at Temperatures from 50 to 500 K , 2000 .
[30] W. B. Johnston,et al. Band parameters and k coefficients for self-broadened ammonia in the range 4000-11,000 cm -1 . , 1999 .
[31] D. Hunten,et al. Helium in Jupiter's atmosphere: Results from the Galileo probe Helium Interferometer Experiment , 1998 .
[32] E. Karkoschka. Spectrophotometry of the Jovian Planets and Titan at 300- to 1000-nm Wavelength: The Methane Spectrum , 1994 .
[33] Giovanni Buffa,et al. N2, O2, H2, Ar and He broadening in the ν1 band of NH3 , 1993 .
[34] Alan S. Pine,et al. Self broadening in the v1 band of NH3 , 1993 .
[35] A. Lacis,et al. A description of the correlated k distribution method for modeling nongray gaseous absorption, thermal emission, and multiple scattering in vertically inhomogeneous atmospheres , 1991 .
[36] Y. Yung,et al. Atmospheric Radiation: Theoretical Basis , 1989 .
[37] Lothar Frommhold,et al. Collision-induced infrared spectra of H2-He pairs at temperatures from 18 to 7000 K. II - Overtone and hot bands , 1989 .
[38] C. E. Keffer,et al. Pressure broadening of ammonia lines in the 6475åband at room and low temperatures , 1986 .
[39] Wm. Hayden Smith,et al. Hydrogen broadening of vibrational-rotational transitions of ammonia lying near 6450 Å , 1985 .
[40] L. Giver,et al. A laboratory atlas of the 5ν1 NH3 absorption band at 6475 Å with applications to Jupiter and Saturn , 1975 .
[41] J. Hansen,et al. Light scattering in planetary atmospheres , 1974 .
[42] G. Plass,et al. Matrix operator theory of radiative transfer. 1: rayleigh scattering. , 1973, Applied optics.
[43] J. Hansen. Multiple Scattering of Polarized Light in Planetary Atmospheres Part II. Sunlight Reflected by Terrestrial Water Clouds , 1971 .
[44] R. Goody,et al. A statistical model for water‐vapour absorption , 1952 .
[45] R. Garland. Modelling the Spectra of Brown Dwarfs , 2018 .
[46] S. Calcutt,et al. Analysis of gaseous ammonia (NH 3 ) absorption in the visible spectrum of Jupiter , 2017 .
[47] M. R. Cherkasov. Broadening and collisional interference of lines in the IR spectra of ammonia: Self-broadening in the ν1 band , 2017 .
[48] Laurence S. Rothman,et al. H2, He, and CO2 line-broadening coefficients, pressure shifts and temperature-dependence exponents for the HITRAN database. Part 1: SO2, NH3, HF, HCl, OCS and C2H2 , 2016 .
[49] E. R. Polovtseva,et al. The HITRAN2012 molecular spectroscopic database , 2013 .
[50] Michael Wegner,et al. Ground-based and Airborne Instrumentation for Astronomy III , 2010 .
[51] M. Sheik-Bahae. NONLINEAR OPTICS, BASICS | Kramers–Krönig Relations in Nonlinear Optics , 2005 .
[52] A. Borysow,et al. Modeling of Collision-Induced Infrared Absorption Spectra of H2 Pairs in the First Overtone Band at Temperatures from 20 to 500 K , 1995 .
[53] Lothar Frommhold,et al. Collision-induced infrared spectra of H2-He pairs involving 0-1 vibrational transitions and temperatures from 18 to 7000 K , 1989 .
[54] K. Lehmann,et al. Spectroscopy and intramolecular dynamics of highly excited vibrational states of NH3 , 1988 .
[55] T. Owen,et al. The visible bands of ammonia - Band strengths, curves of growth, and the spatial distribution of ammonia on Jupiter , 1980 .
[56] V. Oinas,et al. Atmospheric Radiation , 1963, Nature.