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Simulating the one‐dimensional structure of Titan's upper atmosphere: 3. Mechanisms determining methane escape
dc.contributor.authorBell, Jared M.en_US
dc.contributor.authorBougher, Stephen W.en_US
dc.contributor.authorWaite, J. Hunteren_US
dc.contributor.authorRidley, Aaron J.en_US
dc.contributor.authorMagee, Brian A.en_US
dc.contributor.authorMandt, Kathleen E.en_US
dc.contributor.authorWestlake, Josephen_US
dc.contributor.authorDeJong, Anna D.en_US
dc.contributor.authorBar‐nun, Akivaen_US
dc.contributor.authorJacovi, Ronenen_US
dc.contributor.authorToth, Gaboren_US
dc.contributor.authorDe La Haye, Virginieen_US
dc.contributor.authorGell, Daviden_US
dc.contributor.authorFletcher, Gregoryen_US
dc.date.accessioned2013-01-03T19:34:23Z
dc.date.available2013-01-03T19:34:23Z
dc.date.issued2011-11en_US
dc.identifier.citationBell, Jared M.; Bougher, Stephen W.; Waite, J. Hunter; Ridley, Aaron J.; Magee, Brian A.; Mandt, Kathleen E.; Westlake, Joseph; DeJong, Anna D.; Bar‐nun, Akiva ; Jacovi, Ronen; Toth, Gabor; De La Haye, Virginie; Gell, David; Fletcher, Gregory (2011). "Simulating the oneâ dimensional structure of Titan's upper atmosphere: 3. Mechanisms determining methane escape." Journal of Geophysical Research: Planets 116(E11): n/a-n/a. <http://hdl.handle.net/2027.42/94596>en_US
dc.identifier.issn0148-0227en_US
dc.identifier.issn2156-2202en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/94596
dc.publisherWiley Periodicals, Inc.en_US
dc.publisherSpringeren_US
dc.subject.otherThermosphereen_US
dc.subject.otherIonosphereen_US
dc.subject.otherDynamicsen_US
dc.subject.otherTitanen_US
dc.titleSimulating the one‐dimensional structure of Titan's upper atmosphere: 3. Mechanisms determining methane escapeen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/94596/1/jgre2822.pdf
dc.identifier.doi10.1029/2010JE003639en_US
dc.identifier.sourceJournal of Geophysical Research: Planetsen_US
dc.identifier.citedreferenceSchunk, R., and A. F. Nagy ( 2000 ), Ionospheres, Cambridge Univ. Press, Cambridge, U. K.en_US
dc.identifier.citedreferenceAtreya, S. K. ( 1986 ), Atmospheres and Ionospheres of the Outer Planets and Their Satellites, Phys. Chem. Space, vol. 15, Springer, Berlin.en_US
dc.identifier.citedreferenceBar‐Nun, A., V. Dimitrov, and M. Tomasko ( 2008 ), Titan's aerosols: Comparison between our model and DISR findings, Planet. Space Sci., 56, 708 – 714, doi: 10.1016/j.pss.2007.11.014.en_US
dc.identifier.citedreferenceBell, J. M., et al. ( 2010 a), Simulating the one‐dimensional structure of Titan's upper atmosphere: 1. Formulation of the Titan Global Ionosphere‐Thermosphere Model and benchmark simulations, J. Geophys. Res., 115, E12002, doi: 10.1029/2010JE003636.en_US
dc.identifier.citedreferenceBell, J. M., et al. ( 2010 b), Simulating the one‐dimensional structure of Titan's upper atmosphere: 2. Alternative scenarios for methane escape, J. Geophys. Res., 115, E12018, doi: 10.1029/2010JE003638.en_US
dc.identifier.citedreferenceBell, J. M., J. Westlake, and J. H. Waite Jr. ( 2011 ), Simulating the time‐dependent response of Titan's upper atmosphere to periods of magnetospheric forcing, Geophys. Res. Lett., 38, L06202, doi: 10.1029/2010GL046420.en_US
dc.identifier.citedreferenceCrary, F. J., H. T. Smith, D. Reisenfeld, and D. T. Young ( 2010 ), Upper limits on carbon group ions near the orbit of Titan: Implications for methane escape from Titan, paper presented at the 38th Scientific Assembly, Comm. on Space Res., Bremen, Germany, 15 – 18 July.en_US
dc.identifier.citedreferenceDe La Haye, V., J. H. Waite, T. E. Cravens, I. P. Robertson, and S. Lebonnois ( 2008 ), Coupled ion and neutral rotating model of Titan's upper atmosphere, Icarus, 197, 110 – 136, doi: 10.1016/j.icarus.2008.03.022.en_US
dc.identifier.citedreferenceDeng, Y., A. D. Richmond, A. J. Ridley, and H.‐L. Liu ( 2008 ), Assessment of the non‐hydrostatic effect on the upper atmosphere using a general circulation model (GCM), Geophys. Res. Lett., 35, L01104, doi: 10.1029/2007GL032182.en_US
dc.identifier.citedreferenceFulchignoni, M., et al. ( 2005 ), In situ measurements of the physical characteristics of Titan's environment, Nature, 438, 785 – 791, doi: 10.1038/nature04314.en_US
dc.identifier.citedreferenceHunten, D. M. ( 1973 ), The escape of H 2 from Titan, J. Atmos. Sci., 30, 726 – 732.en_US
dc.identifier.citedreferenceKrasnopolsky, V. A. ( 2009 ), A photochemical model of Titan's atmosphere and ionosphere, Icarus, 201, 226 – 256, doi: 10.1016/j.icarus.2008.12.038.en_US
dc.identifier.citedreferenceKrasnopolsky, V. A. ( 2010 ), The photochemical model of Titan's atmosphere and ionosphere: A version without hydrodynamic escape, Planet. Space Sci., 58, 1507 – 1515, doi: 10.1016/j.pss.2010.07.010.en_US
dc.identifier.citedreferenceLiang, M.‐C., A. N. Heays, B. R. Lewis, S. T. Gibson, and Y. L. Yung ( 2007 a), Source of nitrogen isotope anomaly in HCN in the atmosphere of Titan, Astrophys. J., 664, L115 – L118, doi: 10.1086/520881.en_US
dc.identifier.citedreferenceLiang, M.‐C., Y. L. Yung, and D. E. Shemansky ( 2007 b), Photolytically generated aerosols in the mesosphere and thermosphere of Titan, Astrophys. J., 661, L199 – L202, doi: 10.1086/518785.en_US
dc.identifier.citedreferenceMagee, B. A., J. H. Waite, K. E. Mandt, J. Westlake, J. Bell, and D. A. Gell ( 2009 ), INMS‐derived composition of Titan's upper atmosphere: Analysis methods and model comparison, Planet. Space Sci., 57, 1895 – 1916, doi: 10.1016/j.pss.2009.06.016.en_US
dc.identifier.citedreferenceMandt, K. E., J. H. Waite, W. Lewis, B. Magee, J. Bell, J. Lunine, O. Mousis, and D. Cordier ( 2009 ), Isotopic evolution of the major constituents of Titan's atmosphere based on Cassini data, Planet. Space Sci., 57, 1917 – 1930, doi: 10.1016/j.pss.2009.06.005.en_US
dc.identifier.citedreferenceNiemann, H. B., et al. ( 2005 ), The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probe, Nature, 438, 779 – 784, doi: 10.1038/nature04122.en_US
dc.identifier.citedreferenceNiemann, H. B., S. K. Atreya, J. E. Demick, D. Gautier, J. A. Haberman, D. N. Harpold, W. T. Kasprzak, J. I. Lunine, T. C. Owen, and F. Raulin ( 2010 ), The composition of Titan's lower atmosphere and simple surface volatiles as measured by the Cassini‐Huygens probe gas chromatograph mass spectrometer experiment, J. Geophys. Res., 115, E12006, doi: 10.1029/2010JE003659.en_US
dc.identifier.citedreferenceSmith, H. T., R. E. Johnson, M. E. Perry, A. M. Rymer, and T. A. Cassidy ( 2009 ), The influence of neutrals on Saturn's magnetosphere, paper presented at Magnetospheres of the Outer Planets, Univ. of Cologne, Cologne, Germany, 27 – 31 July.en_US
dc.identifier.citedreferenceStrobel, D. F. ( 2008 ), Titan's hydrodynamically escaping atmosphere, Icarus, 193, 588 – 594, doi: 10.1016/j.icarus.2007.08.014.en_US
dc.identifier.citedreferenceStrobel, D. F. ( 2009 ), Titan's hydrodynamically escaping atmosphere: Escape rates and the structure of the exobase region, Icarus, 202, 632 – 641, doi: 10.1016/j.icarus.2009.03.007.en_US
dc.identifier.citedreferenceStrobel, D. F. ( 2010 ), Molecular hydrogen in Titan's atmosphere: Implications of the measured tropospheric and thermospheric mole fractions, Icarus, 208, 878 – 886, doi: 10.1016/j.icarus.2010.03.003.en_US
dc.identifier.citedreferenceTeanby, N. A., et al. ( 2007 ), Vertical profiles of HCN, HC 3 N, and C 2 H 2 in Titan's atmosphere derived from Cassini/CIRS data, Icarus, 186, 364 – 384, doi: 10.1016/j.icarus.2006.09.024.en_US
dc.identifier.citedreferenceTian, F., J. F. Kasting, H. Liu, and R. G. Roble ( 2008 ), Hydrodynamic planetary thermosphere model: 1. Response of the Earth's thermosphere to extreme solar EUV conditions and the significance of adiabatic cooling, J. Geophys. Res., 113, E05008, doi: 10.1029/2007JE002946.en_US
dc.identifier.citedreferenceTucker, O. J., and R. E. Johnson ( 2009 ), Thermally driven atmospheric escape: Monte Carlo simulations for Titan's atmosphere, Planet. Space Sci., 57, 1889 – 1894, doi: 10.1016/j.pss.2009.06.003.en_US
dc.identifier.citedreferenceVervack, R. J., B. R. Sandel, and D. F. Strobel ( 2004 ), New perspectives on Titan's upper atmosphere from a reanalysis of the Voyager 1 UVS solar occultations, Icarus, 170, 91 – 112, doi: 10.1016/j.icarus.2004.03.005.en_US
dc.identifier.citedreferenceWaite, J. H., et al. ( 2004 ), The Cassini Ion and Neutral Mass Spectrometer (INMS) investigation, Space Sci. Rev., 114, 113 – 231, doi: 10.1007/s11214‐004‐1408‐2.en_US
dc.identifier.citedreferenceWilson, E. H., and S. K. Atreya ( 2004 ), Current state of modeling the photochemistry of Titan's mutually dependent atmosphere and ionosphere, J. Geophys. Res., 109, E06002, doi: 10.1029/2003JE002181.en_US
dc.identifier.citedreferenceYelle, R. V., J. Cui, and I. C. F. Müller‐Wodarg ( 2008 ), Methane escape from Titan's atmosphere, J. Geophys. Res., 113, E10003, doi: 10.1029/2007JE003031.en_US
dc.identifier.citedreferenceYung, Y. L., M. Allen, and J. P. Pinto ( 1984 ), Photochemistry of the atmosphere of Titan: Comparison between model and observations, Astrophys. J. Suppl. Ser., 55, 465 – 506, doi: 10.1086/190963.en_US
dc.identifier.citedreferenceAchterberg, R. K., B. J. Conrath, P. J. Gierasch, F. M. Flasar, and C. A. Nixon ( 2008 ), Titan's middle‐atmospheric temperatures and dynamics observed by the Cassini Composite Infrared Spectrometer, Icarus, 194, 263 – 277, doi: 10.1016/j.icarus.2007.09.029.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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