The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail

As a sequence of Ugai (2010b), the present paper studies in detail the structure and dynamics of large-scale (principal) plasmoid, generated by the fast reconnection evolution in a sheared current sheet with no initial northward field component. The overall plasmoid domain is divided into the...

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Main Author: M. Ugai
Format: Article
Language:English
Published: Copernicus Publications 2011-01-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/29/147/2011/angeo-29-147-2011.pdf
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spelling doaj-f3356183eebd4959add1adbe495baf982020-11-25T00:49:08ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762011-01-012914715610.5194/angeo-29-147-2011The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tailM. Ugai0Research Center for Space and Cosmic Evolution, Ehime University, Matsuyama 790-8577, JapanAs a sequence of Ugai (2010b), the present paper studies in detail the structure and dynamics of large-scale (principal) plasmoid, generated by the fast reconnection evolution in a sheared current sheet with no initial northward field component. The overall plasmoid domain is divided into the plasmoid reconnection region P and the plasmoid core region C. In the region P, the magnetized plasma with reconnected field lines are accumulated, whereas in the region C, the plasma, which was intially embedded in the current sheet and has been ejected away by the reconnection jet, is compressed and accumulated. In the presence of the sheared magnetic field in the east-west direction in the current sheet, the upper and lower parts of the reconnection region P are inversely shifted in the east-west directions. Accordingly, the plasmoid core region C with the accumulated sheared field lines is bent in the north-south direction just ahead of the plasmoid center <I>x</I>=</I>X</I><sub>C</sub>, causing the magnetic field component in the north-south direction, whose sign is always opposite to that of the reconnected field lines. Therefore, independently of the sign of the initial sheared field, the magnetic field component <I>B</I><sub>z</sub> in the north-south direction has the definite bipolar profile around <I>X</I><sub>C</sub> along the x-axis. At <I>x</I>=<I>X</I><sub>C</sub>, the sheared field component has the peak value, and as the sheared fields accumulated in the region C become larger, the bipolar field profile becomes more distinct.https://www.ann-geophys.net/29/147/2011/angeo-29-147-2011.pdf
collection DOAJ
language English
format Article
sources DOAJ
author M. Ugai
spellingShingle M. Ugai
The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail
Annales Geophysicae
author_facet M. Ugai
author_sort M. Ugai
title The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail
title_short The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail
title_full The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail
title_fullStr The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail
title_full_unstemmed The structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail
title_sort structure and dynamics of a large-scale plasmoid generated by fast reconnection in the geomagnetic tail
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2011-01-01
description As a sequence of Ugai (2010b), the present paper studies in detail the structure and dynamics of large-scale (principal) plasmoid, generated by the fast reconnection evolution in a sheared current sheet with no initial northward field component. The overall plasmoid domain is divided into the plasmoid reconnection region P and the plasmoid core region C. In the region P, the magnetized plasma with reconnected field lines are accumulated, whereas in the region C, the plasma, which was intially embedded in the current sheet and has been ejected away by the reconnection jet, is compressed and accumulated. In the presence of the sheared magnetic field in the east-west direction in the current sheet, the upper and lower parts of the reconnection region P are inversely shifted in the east-west directions. Accordingly, the plasmoid core region C with the accumulated sheared field lines is bent in the north-south direction just ahead of the plasmoid center <I>x</I>=</I>X</I><sub>C</sub>, causing the magnetic field component in the north-south direction, whose sign is always opposite to that of the reconnected field lines. Therefore, independently of the sign of the initial sheared field, the magnetic field component <I>B</I><sub>z</sub> in the north-south direction has the definite bipolar profile around <I>X</I><sub>C</sub> along the x-axis. At <I>x</I>=<I>X</I><sub>C</sub>, the sheared field component has the peak value, and as the sheared fields accumulated in the region C become larger, the bipolar field profile becomes more distinct.
url https://www.ann-geophys.net/29/147/2011/angeo-29-147-2011.pdf
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