Jupiter's magnetic field as revealed by the synchrotron radiation belts - I. Comparison of a 3-D reconstruction with models of the field

Astronomy and Astrophysics

Volumn 347, Issue 3, 1999, Pages 1029-1038

  Dulk, G A ^a   Leblanc, Y ^a   Sault, R J ^b   Bolton, S J ^c   Waite, J H ^d   Connerney, J E P ^e  

^a OBSERVATOIRE DE PARIS   (France)

^b CSIRO   (Australia)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d SOUTHWEST RESEARCH INSTITUTE   (United States)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Magnetic fields; Planets and satellites: individual: Jupiter; Plasmas; Radiation mechanisms: non thermal; Radio continuum: solar system

Indexed keywords

EID: 0004785518     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (5)

1. Connerney. J.E.P., 1992, In: H.O. Rucker, S.J. Bauer eds., Planetary Radio Emissions III, Austrian Academy of Sciences, p. 13
2. Connerney, J.E.P., 1993, J. Geophys. Res., 98, 18659
3. Connerney, J.E.P., Acuna, M.H., Ness, N.F., Satoh, T., 1998, J. Geophys. Res., 103, 11929
4. de Pater, I., 1981a, J. Geophys. Res., 86, 3397
5. de Pater, I., 1981b, J. Geophys, Res., 86, 3423