Morphology of the magnetic field near Titan: Hybrid model study of the Cassini T9 flyby

Geophysical Research Letters

Volumn 34, Issue 24, 2007, Pages

  Kallio, Esa ^a   Sillanpaa I ^a   Jarvinen, R ^a   Janhunen, P ^a   Dougherty, M ^b   Bertucci, C ^b   Neubauer, F ^c  

^a FINNISH METEOROLOGICAL INSTITUTE   (Finland)

^b IMPERIAL COLLEGE LONDON   (United Kingdom)

^c UNIVERSITY OF COLOGNE   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

DEFORMATION; IONS; MAGNETIC FIELDS; MATHEMATICAL MODELS; MORPHOLOGY; PLASMAS; SATELLITES; SPACE FLIGHT;

SUB-ROTATING PLASMA; WING-LIKE FLUX TUBE;

GEOMAGNETISM;

MAGNETIC FIELD; MORPHOLOGY; NUMERICAL MODEL; SATELLITE MISSION; TITAN;

EID: 39549117385     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2007GL030827     Document Type: Article

References (9)

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2. Coates, A. J., F. J. Crary, D. T. Young, K. Szego, C. S. Arridge, Z. Bebesi, E. C. Sittler Jr., R. E. Hartle, and T. W. Hill (2007), Ionospheric electrons in Titan's tail: Plasma structure during the Cassini T9 encounter, Geophys. Res. Lett., 34, L24S05, doi:10.1029/ 2007GL030919.
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