For the March/April 1991 time period, the alpha/proton abundance ratio, the proton kinetic temperature and speed distributions, and the relative abundance of O(+7) to O(+6) is determined over each 13-minute duty cycle of the Solar Wind Ion Composition Spectrometer (SWICs) experiment on Ulysses. The ratio O(+7)/O(+6) (as a relative measure of ionization temperature) is shown to be useful in identifying possible coronal mass ejection (CME) events. We report measurements of silicon/oxygen abundance ratios and silicon and oxygen charge state distributions in the solar wind during a CME event and compare these compositions to a 'normal' solar wind time period.


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    Titel :

    Solar wind composition measurements by the Ulysses SWICS experiment during transient solar wind flows


    Beteiligte:
    Galvin, A. B. (Autor:in) / Gloeckler, G. (Autor:in) / Ipavich, F. M. (Autor:in) / Shafer, C. M. (Autor:in) / Geiss, J. (Autor:in) / Ogilvie, K. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.06.1993



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :



    Solar wind composition measurements by the Ulysses SWICS experiment during transient solar wind flows

    Galvin, A.B. / Gloeckler, G. / Ipavich, F.M. et al. | Elsevier | 1993



    Sulfur abundances in the solar wind measured by SWICS on Ulysses

    Shafer, C. M. / Gloeckler, G. / Galvin, A. B. et al. | NTRS | 1993


    Sulfur abundances in the solar wind measured by SWICS on Ulysses

    Shafer, C.M. / Gloeckler, G. / Galvin, A.B. et al. | Elsevier | 1993