Longitudinal modulation of the brightness of Io's auroral footprint emission: Comparison with models

Author:

Wannawichian S.12,Clarke J. T.3,Bagenal F.4,Smyth W. H.56,Peterson C. A.5,Nichols J. D.7

Affiliation:

1. Department of Physics and Materials Science, Faculty of Science; Chiang Mai University; Chiang Mai Thailand

2. ThEP Center; CHE; Bangkok Thailand

3. Center for Space Physics; Boston University; Boston Massachusetts USA

4. Department of Astrophysical and Planetary Sciences and Laboratory for Atmospheric and Space Physics; University of Colorado; Boulder Colorado USA

5. Atmospheric and Environmental Research, Inc.; Lexington Massachusetts USA

6. Deceased 30 September 2011

7. Department of Physics and Astronomy; University of Leicester; Leicester UK

Funder

NASA

Space Telescope Science Institute to Boston University

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference50 articles.

1. The main magnetic field of Jupiter;Acuña;J. Geophys. Res.,1976

2. Empirical model of the Io plasma torus: Voyager measurement;Bagenal;J. Geophys. Res.,1994

3. Dawn-dusk electric field asymmetry of the Io plasma torus;Barbosa;J. Geophys. Res.,1983

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

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