On the sources of Jovian hectometric radiation

F. Nakagawa, A. Morioka, H. Misawa

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)

Abstract

Jovian hectometric radiation(HOM) emitted from the polar region of the Jovian magnetsphere reflects the information on the electro-magnetic environment of the source region. Using the Ulysses URAP and SWOOPS data, the occurrence characteristics of HOM and its relation to the solar wind were investigated. As a result, we found that HOM can be classified into two components; (1) Solar wind HOM(sw-HOM), whose amplitudes are related to the solar wind dynamic pressure, and (2) non Solar wind HOM(nsw-HOM), which is independent to the solar wind parameters and is observed with large amplitudes. These two components have different system III occurrence characteristics. Considering the relationship with Jovian aurora, L values of each HOM source are inferred to be L>30, L≃12, respectively.

Original languageEnglish
Pages (from-to)1541-1544
Number of pages4
JournalAdvances in Space Research
Volume26
Issue number10
DOIs
Publication statusPublished - 2000 Jan 1

ASJC Scopus subject areas

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

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