An improved solution to the “Rankine‐Hugoniot” problem
- 1 August 1994
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 99 (A8) , 14737-14746
- https://doi.org/10.1029/94ja00782
Abstract
This paper presents an extension of the nonlinear least squares fitting technique of Viñas and Scudder [1986] (VS), which finds the physical and geometrical properties of nondissipational magnetohydrodynamic (MHD) shocks. The new method incorporates plasma temperature observations in the form of normal momentum flux and energy density flux conservation as well as plasma density, velocity, and magnetic field data. The new technique is capable of using known standard deviations in the individual measurement points to properly weight the fitting procedure. The new fitting code is validated through the analysis of synthetic shocks with known physical and geometrical properties. Finally, it is compared to the original VS method and the preaveraged velocity coplanarity technique.Keywords
This publication has 7 references indexed in Scilit:
- Plasma Observations Near Neptune: Initial Results from Voyager 2Science, 1989
- The Uranian bow shock: Voyager 2 inbound observations of a high Mach number shockJournal of Geophysical Research, 1987
- Fast and optimal solution to the “Rankine‐Hugoniot problem”Journal of Geophysical Research, 1986
- The plasma experiment on the 1977 Voyager MissionSpace Science Reviews, 1977
- Interplanetary shocks seen by Ames Plasma Probe on Pioneer 6 and 7Journal of Geophysical Research, 1976
- Determination of magnetohydrodynamic shock normalsJournal of Geophysical Research, 1972
- Single spacecraft method of estimating shock normalsJournal of Geophysical Research, 1971