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Cassini measurements of cold plasma in the ionosphere of Titan.
Wahlund, J E; Boström, R; Gustafsson, G; Gurnett, D A; Kurth, W S; Pedersen, A; Averkamp, T F; Hospodarsky, G B; Persoon, A M; Canu, P; Neubauer, F M; Dougherty, M K; Eriksson, A I; Morooka, M W; Gill, R; André, M; Eliasson, L; Müller-Wodarg, I.
Afiliación
  • Wahlund JE; Swedish Institute of Space Physics, Box 537, SE-751 21 Uppsala, Sweden. jwe@irfu.se
Science ; 308(5724): 986-9, 2005 May 13.
Article en En | MEDLINE | ID: mdl-15894529
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.
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Colección: 01-internacional Base de datos: MEDLINE Asunto principal: Saturno Idioma: En Revista: Science Año: 2005 Tipo del documento: Article País de afiliación: Suecia Pais de publicación: Estados Unidos
Buscar en Google
Colección: 01-internacional Base de datos: MEDLINE Asunto principal: Saturno Idioma: En Revista: Science Año: 2005 Tipo del documento: Article País de afiliación: Suecia Pais de publicación: Estados Unidos