Grad-Shafranov reconstruction of magnetic clouds: overview and improvements
Abstract
The Grad-Shafranov reconstruction is a method of estimating the orientation (invariant axis) and cross-section of magnetic flux ropes using the data from a single spacecraft. It can be applied to various magnetic structures such as magnetic clouds (MCs) and flux ropes embedded into the magnetopause and in the solar wind. We develop a number of improvements of this technique and show some examples of the reconstruction procedure of interplanetary coronal mass ejections (ICMEs) observed at 1 AU by the STEREO, WIND and ACE spacecraft during the minimum following the solar cycle 23. The analysis is conducted not only for ideal localized ICME events but also for non-trivial cases of magnetic clouds in fast solar wind. The Grad-Shafranov reconstruction gives reasonable results for the sample events, although it possesses certain limitations, which need to be taken into account during the interpretation of the model results.
Keywords
Cite
@article{arxiv.1108.1678,
title = {Grad-Shafranov reconstruction of magnetic clouds: overview and improvements},
author = {Alexey Isavnin and Emilia K. J. Kilpua and Hannu E. J. Koskinen},
journal= {arXiv preprint arXiv:1108.1678},
year = {2012}
}
Comments
16 pages, 13 figures