Number of the records: 1  

A diffusive equilibrium model for the plasma density in Saturn's magnetosphere

  1. 1.
    SYSNO ASEP0332598
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleA diffusive equilibrium model for the plasma density in Saturn's magnetosphere
    TitleModel difuzní rovnováhy pro hustotu plazmatu v magnetosféře Saturnu
    Author(s) Persoon, A. M. (US)
    Gurnett, D. A. (US)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Kurth, W. S. (US)
    Faden, J. B. (US)
    Groene, J. B. (US)
    Lewis, G. R. (GB)
    Coates, A. J. (GB)
    Wilson, R. J. (US)
    Tokar, L. R. (US)
    Wahlund, J.-E. (SE)
    Moncuquet, M. (FR)
    Source TitleJournal of Geophysical Research - ISSN 0148-0227
    Roč. 114, - (2009), A04211/1-A04211/19
    Number of pages19 s.
    Languageeng - English
    CountryUS - United States
    Keywordsdiffusive equilibrium ; Saturn's magnetosphere ; Cassini spacecraft
    Subject RIVBL - Plasma and Gas Discharge Physics
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    UT WOS000265675600006
    DOI10.1029/2008JA013912
    AnnotationElectron density measurements have been obtained by the Cassini Radio and Plasma Wave Science (RPWS) instrument for more than 50 passes through Saturn’s inner magnetosphere from 30 June 2004 to 30 September 2007. The electron densities are derived from RPWS measurements of the upper hybrid resonance frequency and span latitudes up to 35 and L values from 3.6 to 10. The electron density measurements are combined with ion anisotropy measurements from the Cassini Plasma Spectrometer (CAPS) and electron temperature measurements from the RPWS and CAPS to develop a diffusive equilibrium model for the distribution of water group ions, hydrogen ions, and electrons in the inner region of Saturn’s magnetosphere. The model uses an analytical solution of the field-aligned force equation, including the ambipolar electric field, to determine the equatorial ion densities and scale heights as a function of L. Density contour plots for water group ions, hydrogen ions, and electrons are presented
    WorkplaceInstitute of Atmospheric Physics
    ContactKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Year of Publishing2010
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.