Asset Publisher

Grad-Shafranov Reconstruction of Magnetic Flux Ropes in the Near-Earth Space

Grad-Shafranov Reconstruction of Magnetic Flux Ropes in the Near-Earth Space

Publication date: 23 April 2011

Authors: Lui, A.T.Y.

Journal: Space Sci. Rev.
Year: 2011

Copyright: Springer

Electric currents permeate space plasmas and often have a significant component along the magnetic field to form magnetic flux ropes. A larger spatial perspective of these structures than from the direct observation along the satellite path is crucial in visualizing their role in plasma dynamics. For magnetic flux ropes that are approximately two-dimensional equilibrium structures on a certain plane, Grad-Shafranov reconstruction technique, developed by Bengt Sonnerup and his colleagues (see Sonnerup et al. in J. Geophys. Res. 111:A09204, 2006), can be used to reveal two-dimensional maps of associated plasma and field parameters. This review gives a brief account of the technique and its application to magnetic flux ropes near the Earth's magnetopause, in the solar wind, and in the magnetotail. From this brief survey, the ranges of the total field-aligned current and the total magnetic flux content for these magnetic flux ropes are assessed. The total field-aligned current is found to range from ~0.14 to ~9.7×104 MA, a range of nearly six orders of magnitude. The total magnetic flux content is found to range from ~0.25 to ~2.3×106 MWb, a range of nearly seven orders of magnitude. To the best of our knowledge, this review reports the largest range of both the total field-aligned current and the total magnetic flux content for magnetic flux ropes in space plasmas.

Link to publication
Last Update: Sep 1, 2019 8:56:24 AM
28-Nov-2021 19:59 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/ApP6bLA

Images And Videos

Related Publications

Related Links

See Also

Documentation