Modified ``Rankine-Hugoniot'' shock fitting technique: Simultaneous solution for shock normal and speed

Details Modified ``Rankine-Hugoniot'' shock fitting technique: Simultaneous solution for shock normal and speed Modified ``Rankine-Hugoniot'' shock fitting technique: Simultaneous solution for shock normal and speed

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jgra..11310110k&link_type=abstract

Journal of Geophysical Research, Volume 113, Issue A10, CiteID A10110

Physics

Plasma Physics

3

Interplanetary Physics: Interplanetary Shocks, Space Plasma Physics: Mathematical And Numerical Techniques (0500, 3200), Space Plasma Physics: Shock Waves (4455), Space Plasma Physics: Discontinuities (2109)

Scientific paper

We introduce a modification of the nonlinear least squares fitting technique of Viñas and Scudder and Szabo (VSSz) with simultaneous determination of the shock normal direction ($\theta$ and $\phi$) and propagation speed (V S ). Similar to the 2D case of the VSSz technique, the uniqueness of the solution can still be graphically demonstrated in the 3D space of the unknown variables. The modified technique is validated through the analysis of synthetic shocks and is also applied to an interplanetary shock observed by Wind. Our technique provides self-consistent 3D confidence regions for the parameters while the VSSz technique assumes the independence of the V S confidence interval from $\theta$ and $\phi$. The 3D confidence region is highly dependent on V S resulting in $\theta$ and $\phi$ joint confidence regions that are generally significantly larger and oriented differently than those obtained by the VSSz technique. This also leads to significantly larger confidence intervals for the individual parameters determined by our modified technique. While the best fit values provided by the two techniques are usually close to each other, we also demonstrate the advantage of the V S best fit value determination with our technique in the case when a small density jump is combined with significant density fluctuations. The agreement between the best fit solutions of the techniques can also be used as a test for the correctness of the chosen upstream and downstream intervals.

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