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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 29, issue 11
Ann. Geophys., 29, 2081–2088, 2011
https://doi.org/10.5194/angeo-29-2081-2011
© Author(s) 2011. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue: Dynamical processes in space plasmas

Ann. Geophys., 29, 2081–2088, 2011
https://doi.org/10.5194/angeo-29-2081-2011
© Author(s) 2011. This work is distributed under
the Creative Commons Attribution 3.0 License.

Regular paper 22 Nov 2011

Regular paper | 22 Nov 2011

Spatial scales of the magnetic ramp at the Venusian bow shock

A. P. Dimmock1, S. N. Walker1, T. L. Zhang2, and S. A. Pope1 A. P. Dimmock et al.
  • 1Automatic Control & Systems Engineering, University of Sheffield, Sheffield, UK
  • 2Space Research Institute of Austrian Academy of Sciences, Graz, Austria

Abstract. Typically multi-spacecraft missions are ideally suited to the study of shock spatial scales due to the separation of temporal and spatial variations. These missions are not possible at all locations and therefore in-situ multi-spacecraft measurements are not available beyond the Earth. The present paper presents a study of shock spatial scales using single spacecraft measurements made by the Venus Express spacecraft. The scales are determined based on previous knowledge of shock overshoot scales measured by the ISEE and Cluster missions. The study encompasses around 60 crossings of the Venusian bow shock from 2006 to 2009. The statistical relationship between the shock ramp spatial scales, overshoot and upstream shock parameters are investigated. We find that despite somewhat different solar wind conditions our results are comparable with those based on multi-spacecraft missions at the terrestrial bow shock.

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