Model of the Jovian magnetic field topology constrained by the Io auroral emissions

Author:

Hess S. L. G.1,Bonfond B.2,Zarka P.3,Grodent D.2

Affiliation:

1. LASP; University of Colorado at Boulder; Boulder Colorado USA

2. LPAP; Université de Liège; Liège Belgium

3. LESIA; Observatoire de Paris-CNRS; Meudon France

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference55 articles.

1. The Pioneer XI high field fluxgate magnetometer;Acuna;Space Sci. Instrum.,1975

2. Jupiter's main magnetic field measured by Pioneer 11;Acuna;Nature,1975

3. Magnetic field experiment for Voyagers 1 and 2;Behannon;Space Sci. Rev.,1977

4. Influence of the satellite Io on Jupiter's decametric emission;Bigg;Nature,1964

5. Radio Jupiter after Voyager: An overview of the planetary radio astronomy observations;Boischot;J. Geophys. Res.,1981

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