Grad-Shafranov Reconstruction Technique and Its Applications

Details Grad-Shafranov Reconstruction Technique and Its Applications Grad-Shafranov Reconstruction Technique and Its Applications

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..221h&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 221-228 (2004).

Physics

1

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Interplanetary Magnetic Fields

Scientific paper

The Grad-Shafranov reconstruction technique involves the Grad-Shafranov equation governing 2 12 dimensional structures, and the magnetic and plasma measurements from a single spacecraft. It is capable of deriving, quantitatively, a 2D cross section characterizing non-axisymmetric, cylindrical magnetic structures. Its applications to observations in the inner heliosphere, such as the magnetic flux ropes observed by spacecraft WIND and ACE, are reported. Multi-spacecraft validation and its application to structures beyond 1 AU are discussed.

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