BIROn - Birkbeck Institutional Research Online

    Saturn's auroral/polar H3+infrared emission: the effect of solar wind compression

    Stallard, T.S. and Masters, A. and Miller, Steve and Melin, H. and Bunce, E.J. and Arridge, Chris S. and Achilleos, Nick and Dougherty, M.K. and Cowley, S.W.H. (2012) Saturn's auroral/polar H3+infrared emission: the effect of solar wind compression. Journal of Geophysical Research: Space Physics 117 (A12), ISSN 0148-0227.

    Full text not available from this repository.

    Abstract

    Previous investigations into Saturn's aurora have shown that they are strongly controlled by the solar wind. Here, for the first time, we use a combination of ground-based infrared observations of the aurora and in situ measurements of the magnetosphere in order to better understand this association. We show that large-scale variability in both the intensity and ion flow velocities can be directly correlated with the solar wind dynamic pressure, with, in particular, the arrival of solar wind compressions. Large compressions in the solar wind trigger the same morphological changes in the auroral structure as have previously been seen in UV images, and these are accompanied by the loss of the open field line corotation region seen in the velocity measurements. This region has been explained as an “old core” of magnetic field lines open to the solar wind, protected from reconnection due to the twisting in the magnetotail, and therefore requires that this region be removed only by major compressions in the solar wind; thus, our observations here generally agree with this model. In addition, we have observed a >8 h delay between the arrival of a major compression and the resulting effect upon the aurora, suggesting that reconnection must either occur well into the tail or that there are other processes in the chain of events that lead to the major dawn brightening seen in both these observations and previously studied UV images.

    Metadata

    Item Type: Article
    Keyword(s) / Subject(s): H3+, Saturn, atmosphere, aurora, infrared, ionosphere
    School: Birkbeck Faculties and Schools > Faculty of Science > School of Natural Sciences
    Depositing User: Administrator
    Date Deposited: 26 Nov 2014 13:41
    Last Modified: 02 Aug 2023 17:14
    URI: https://eprints.bbk.ac.uk/id/eprint/11122

    Statistics

    Activity Overview
    6 month trend
    0Downloads
    6 month trend
    374Hits

    Additional statistics are available via IRStats2.

    Archive Staff Only (login required)

    Edit/View Item
    Edit/View Item