https://dx.doi.org/https://doi.org/10.5194/angeo-28-491-2010">
 

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Creative Commons Attribution 3.0 License
This work is licensed under a Creative Commons Attribution 3.0 License.

Abstract

STEREO/PLASTIC determines three-dimensional distributions of solar wind iron ions with unprecedented time resolution. Typically 300 to 1000 counts are registered within each 5 min time interval. For the present study we use the information contained in these distributions to characterize CIRs (Corotating Interaction Regions) in two test cases. We perform a consistency test for both the derived physical parameters and for the analytical model of CIRs of Lee (2000). At 1 AU we find that apart from compositional changes the most indicative parameter for marking the time when a CIR passes a spacecraft is the angular deflection of the flow vector of particles. Changes in particle densities and the changes in magnitudes of speeds are apparently less reliable indicators of stream interfaces.

Publication Date

2-9-2010

Journal Title

Annales Geophysicae

Publisher

EGU

Document Type

Article

Comments

This is an article published by EGU in Annales Geophysicae in 2010, available online: https://dx.doi.org/https://doi.org/10.5194/angeo-28-491-2010

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