BIROn - Birkbeck Institutional Research Online

    Cassini multi-instrument assessment of Saturn's polar cap boundary

    Jinks, S.L. and Bunce, E.J. and Cowley, S.W.H. and Provan, G. and Yeoman, T.K. and Arridge, Chris S. and Dougherty, M.K. and Gurnett, D.A. and Krupp, N. and Kurth, W.S. and Mitchell, D.G. and Morooka, M. and Wahlund, J.-E. (2014) Cassini multi-instrument assessment of Saturn's polar cap boundary. Journal of Geophysical Research: Space Physics 119 (10), pp. 8161-8177. ISSN 2169-9380.

    [img]
    Preview
    Text
    11028.pdf - Published Version of Record
    Available under License Creative Commons Attribution.

    Download (3MB) | Preview

    Abstract

    We present the first systematic investigation of the polar cap boundary in Saturn's high-latitude magnetosphere through a multi-instrument assessment of various Cassini in situ data sets gathered between 2006 and 2009. We identify 48 polar cap crossings where the polar cap boundary can be clearly observed in the step in upper cutoff of auroral hiss emissions from the plasma wave data, a sudden increase in electron density, an anisotropy of energetic electrons along the magnetic field, and an increase in incidence of higher-energy electrons from the low-energy electron spectrometer measurements as we move equatorward from the pole. We determine the average level of coincidence of the polar cap boundary identified in the various in situ data sets to be 0.34° ± 0.05° colatitude. The average location of the boundary in the southern (northern) hemisphere is found to be at 15.6° (13.3°) colatitude. In both hemispheres we identify a consistent equatorward offset between the poleward edge of the auroral upward directed field-aligned current region of ~1.5–1.8° colatitude to the corresponding polar cap boundary. We identify atypical observations in the boundary region, including observations of approximately hourly periodicities in the auroral hiss emissions close to the pole. We suggest that the position of the southern polar cap boundary is somewhat ordered by the southern planetary period oscillation phase but that it cannot account for the boundary's full latitudinal variability. We find no clear evidence of any ordering of the northern polar cap boundary location with the northern planetary period magnetic field oscillation phase.

    Metadata

    Item Type: Article
    Keyword(s) / Subject(s): Saturn, magnetosphere, polar cap, high latitude
    School: Birkbeck Schools and Departments > School of Science > Earth and Planetary Sciences > UCL/Birkbeck Centre for Planetary Sciences
    Depositing User: Administrator
    Date Deposited: 19 Nov 2014 17:11
    Last Modified: 28 Jul 2019 23:05
    URI: http://eprints.bbk.ac.uk/id/eprint/11028

    Statistics

    Downloads
    Activity Overview
    117Downloads
    145Hits

    Additional statistics are available via IRStats2.

    Archive Staff Only (login required)

    Edit/View Item Edit/View Item