Ultra-relativistic electrons in Jupiter's radiation belts View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2002-02

AUTHORS

S. J. Bolton, M. Janssen, R. Thorne, S. Levin, M. Klein, S. Gulkis, T. Bastian, R. Sault, C. Elachi, M. Hofstadter, A. Bunker, G. Dulk, E. Gudim, G. Hamilton, W. T. K. Johnson, Y. Leblanc, O. Liepack, R. McLeod, J. Roller, L. Roth, R. West

ABSTRACT

Ground-based observations have shown that Jupiter is a two-component source of microwave radio emission1: thermal atmospheric emission and synchrotron emission2 from energetic electrons spiralling in Jupiter's magnetic field. Later in situ measurements3,4 confirmed the existence of Jupiter's high-energy electron-radiation belts, with evidence for electrons at energies up to 20 MeV. Although most radiation belt models predict electrons at higher energies5,6, adiabatic diffusion theory can account only for energies up to around 20 MeV. Unambiguous evidence for more energetic electrons is lacking. Here we report observations of 13.8 GHz synchrotron emission that confirm the presence of electrons with energies up to 50 MeV; the data were collected during the Cassini fly-by of Jupiter. These energetic electrons may be repeatedly accelerated through an interaction with plasma waves, which can transfer energy into the electrons. Preliminary comparison of our data with model results suggests that electrons with energies of less than 20 MeV are more numerous than previously believed. More... »

PAGES

987-991

References to SciGraph publications

  • 1975. Dénouement of Jovian Radiation Belt Theory in THE MAGNETOSPHERES OF THE EARTH AND JUPITER
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1038/415987a

    DOI

    http://dx.doi.org/10.1038/415987a

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1051011042

    PUBMED

    https://www.ncbi.nlm.nih.gov/pubmed/11875557


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