Wilkinson, William (2001) What the Rankine-Hugoniot relations tell us about co-rotating interaction regions in the solar wind, and what they don't In: Proceedings of the Les Woolliscroft Memorial Conference/Sheffield Space Plasma Meeting: Multi-Point Measurements versus Theory, 24-26 April 2001, Sheffield, UK.Full text not available from this repository.
Co-rotating interaction regions (CIRs) are the result of a fast solar wind streat catching up with a slow stream ahead. The simplest description of a CIR portrays it as a compression region bounded by two fast shock waves. A tangential discontinuity within the CIR separates the shocked fast and slow solar wind streams. In this paper we assume that the Rankine-Hugoniot relations apply across both shocks. These relations are then used to predict the properties of the two shocked plasma states within a set of CIRs observed by the Ulysses spacecraft. The obtained properties are examined for consistency with the simple description of a CIR outlined above and the possible reasons for the observed discrepancies are discussed.
|Item Type:||Contribution to conference proceedings in the public domain ( Full Paper)|
|Subjects:||F000 Physical Sciences > F500 Astronomy|
|Faculties:||Faculty of Science and Engineering > School of Computing, Engineering and Mathematics > Computational Mathematics|
|Depositing User:||Helen Webb|
|Date Deposited:||14 Nov 2007|
|Last Modified:||17 Dec 2015 12:41|
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