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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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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