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Possible two-step solar energy release mechanism due to turbulent magnetic reconnection
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10.1063/1.1862249
/content/aip/journal/pop/12/5/10.1063/1.1862249
http://aip.metastore.ingenta.com/content/aip/journal/pop/12/5/10.1063/1.1862249

Figures

Image of FIG. 1.
FIG. 1.

Time history of the external magnetic reconnection rate , defined by the mean plasma bulk inflow speed far upstream of the current sheet (top, in the unit of ), the maximum outflow velocity along axis in the direction (middle, in the unit of ), and the corresponding observed maximum flux cancellation rate (bottom, in the unit of ).

Image of FIG. 2.
FIG. 2.

Contours of constant , i.e., magnetic field lines at , 50, and 120, respectively (from top to bottom).

Tables

Generic image for table
Table I.

Characteristic values of mentioned physical quantities.

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/content/aip/journal/pop/12/5/10.1063/1.1862249
2005-04-07
2014-04-20
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Possible two-step solar energy release mechanism due to turbulent magnetic reconnection
http://aip.metastore.ingenta.com/content/aip/journal/pop/12/5/10.1063/1.1862249
10.1063/1.1862249
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