1887
banner image
No data available.
Please log in to see this content.
You have no subscription access to this content.
No metrics data to plot.
The attempt to load metrics for this article has failed.
The attempt to plot a graph for these metrics has failed.
Physical conditions for fast reconnection evolution in space plasmas
Rent:
Rent this article for
USD
10.1063/1.4739286
/content/aip/journal/pop/19/7/10.1063/1.4739286
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/7/10.1063/1.4739286
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

Temporal variations of plasma density ρ and current density at the origin for the cases of uniform resistivity , and 0.0003.

Image of FIG. 2.
FIG. 2.

Temporal variations of resistivity η, current density , and electric field at the origin for the Spitzer resistivity model with .

Image of FIG. 3.
FIG. 3.

Temporal variations of plasma density ρ and current density measured at the origin for the anomalous resistivity model.

Image of FIG. 4.
FIG. 4.

Temporal variations of electric field and resistivity η measured at the origin for the anomalous resistivity model.

Image of FIG. 5.
FIG. 5.

Temporal variations of current density measured at the origin for the cases of , and 10 for the anomalous resistivity model in an initially force-free current sheet.

Image of FIG. 6.
FIG. 6.

Temporal variations of relative electron-ion drift velocity measured at the origin with other conditions same as Fig. 5.

Image of FIG. 7.
FIG. 7.

Temporal variations of electric field measured at the origin for the cases of , and 10 for the anomalous resistivity model in an initially force-free current sheet.

Image of FIG. 8.
FIG. 8.

Plasma flow vectors and plasma pressure distributions in the (x, y) plane at times t = 36, 48, and 60 for the anomalous resistivity model in an initially force-free current sheet, where and indicate, respectively, the plasmoid backward end and the plasmoid center.

Image of FIG. 9.
FIG. 9.

Magnetic field lines passing through the x and y axes with other conditions same as Fig. 8.

Image of FIG. 10.
FIG. 10.

Cross section of current sheet like that in the geomagnetic tail, where 2d 0 and 2W indicate its effective thickness and width, respectively.

Loading

Article metrics loading...

/content/aip/journal/pop/19/7/10.1063/1.4739286
2012-07-26
2014-04-16
Loading

Full text loading...

This is a required field
Please enter a valid email address
752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Physical conditions for fast reconnection evolution in space plasmas
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/7/10.1063/1.4739286
10.1063/1.4739286
SEARCH_EXPAND_ITEM