Heating of Minor Ions by the Coronal Slow Shock

Abstract

The coronal slow shock has been changes of alpha particles' velocity, density, and predicted to exist embedded in large coronal holes temperature have been published, both for fast at 4-10 solar radii. We use a three-fluid model to interplanetary shocks and for the Earth's bow study the jumps in minor ion properties across a slow shock such as the coronal… (More)

Topics

5 Figures and Tables

Cite this paper

@inproceedings{Whang2007HeatingOM, title={Heating of Minor Ions by the Coronal Slow Shock}, author={Y. C. Whang and Xuepu Zhao and Kevin Ogilvie}, year={2007} }