Cassini Measurements of Cold Plasma in the Ionosphere of Titan

Author:

Wahlund J.-E.12345,Boström R.12345,Gustafsson G.12345,Gurnett D. A.12345,Kurth W. S.12345,Pedersen A.12345,Averkamp T. F.12345,Hospodarsky G. B.12345,Persoon A. M.12345,Canu P.12345,Neubauer F. M.12345,Dougherty M. K.12345,Eriksson A. I.12345,Morooka M. W.12345,Gill R.12345,André M.12345,Eliasson L.12345,Müller-Wodarg I.12345

Affiliation:

1. Swedish Institute of Space Physics, Box 537, SE-751 21 Uppsala, Sweden.

2. Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA.

3. Department of Physics, University of Oslo, NO-0316 Oslo, Norway.

4. Centre d'Etude des Environnements Terrestre et Planétaires/CNRS/Institut Pierre Simon Laplace, 78140 Vélizy-Villacoublay, France.

5. Institute for Geophysics and Meteorology, Köln University, D-50923 Köln, Germany.

Abstract

The Cassini Radio and Plasma Wave Science (RPWS) Langmuir probe (LP) sensor observed the cold plasma environment around Titan during the first two flybys. The data show that conditions in Saturn's magnetosphere affect the structure and dynamics deep in the ionosphere of Titan. The maximum measured ionospheric electron number density reached 3800 per cubic centimeter near closest approach, and a complex chemistry was indicated. The electron temperature profiles are consistent with electron heat conduction from the hotter Titan wake. The ionospheric escape flux was estimated to be 10 25 ions per second.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference16 articles.

1. Radio and Plasma Wave Observations at Saturn from Cassini's Approach and First Orbit

2. H. Backes et al . paper presented at the American Geophysical Union fall meeting San Francisco 2004.

3. T. E. Cravens et al . in preparation.

4. The Cassini Radio and Plasma Wave Investigation

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