DPS 2001 meeting, November 2001
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All findings are embargoed until the time of presentation at the meeting.


Session 55. Titan II

Oral, Chairs: R. Lorenz, C. Griffith, Saturday,
December 1, 2001, 11:05am-12:35pm, Regency GH

55.01 CO Isotopic Fractionatoin and the Evolution of Early Titan
A. S. Wong, Y. L. Yung, C. G. Morgan (California Institute of Technology), T. Owen (University of Hawaii)
55.02 Titan's 5-micron spectrum: VLT/ISAAC observations
E. Lellouch, A. Coustenis, B. Sebag (Observatoire de Paris), J.-G. Cuby (European Southern Observatory ), J. Crovisier (Observatoire de Paris), J.P. Maillard (I.A.P. Paris)
55.03 Macromolecules and their effects on chemistry and seasonal albedo variations of the Titan haze
E.L.O. Bakes, C.P. McKay, C.W. Bauschlicher, S. Lebonnois (NASA Ames Research Center)
55.04 Mechanisms for the Formation of Haze in the Atmosphere of Titan
E.H. Wilson, S.K. Atreya (University of Michigan at Ann Arbor)
55.05 Radiative lifetime of C4H2*: implications for the atmosphere of Titan
V. Vuitton, M.-C. Gazeau (L.I.S.A., Universités Paris VII et XII, France), C. Gée (Université de Cergy-Pontoise, France), C. Crépin (L.P.P.M., Université Paris-Sud, France), Y. Bénilan (L.I.S.A., Universités Paris VII et XII, France)
55.06 The chemistry of oxygenated compounds in Titan’s atmosphere revisited
P. Coll, J.-M. Bernard, F. Raulin (LISA)
55.07 Latitudinal mixing by barotropic waves in Titan's stratosphere: results from a dynamics-haze-photochemistry GCM
D.M.G.C. Luz (Observatorio Astronomico de Lisboa, Portugal), F. Hourdin (Laboratoire de Meteorologie Dynamique, Paris)
55.08 Changes in Titan's upper atmosphere during solar eclipses
I.C.F. Mueller-Wodarg (University College London and Boston University), R.V. Yelle (Northern Arizona University), M. Mendillo (Boston University), A.D. Aylward (University College London)
55.09 Assimilation of data from the Solar Aureole imager and the Visible Spectrometer onboard the Huygens probe into a radiative transfer model\\of Titan's Atmosphere
B. Grieger (MPIfA)


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