Jupiter's magnetic field as revealed by the synchrotron radiation belts - II. Change of the 2-D brightness distribution with DE

Astronomy and Astrophysics

Volumn 347, Issue 3, 1999, Pages 1039-1045

  Dulk, G A ^a   Leblanc, Y ^a   Sault, R J ^b   Boston, S J ^c  

^a OBSERVATOIRE DE PARIS   (France)

^b CSIRO   (Australia)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

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

Indexed keywords

EID: 1542627468     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (4)

1. Dulk, G.A., Leblanc, Y., Sault, R.J., Ladreiter, H.P., Connerney, J.E., 1997. Astron. Atrophys., 319, 282
2. Dulk, G.A., Leblanc, Y., Sault, R.J., Bolton, S.J., Connerney, J.E.C., 1999. Astron, Astrophys., this issue (Paper I)
3. Leblanc, Y., Dulk, G.A., Sault, R.J., Hunstead, R.W., 1997. Astron. Astrophys., 319, 274
4. Sault, R.J., Oosterloo, T., Dulk, G.A., Leblanc, Y., 1997, Astron. Astrophys., 324, 1190