dc.contributor.author |
Galsgaard, K. |
|
dc.contributor.author |
Rickard, G.J. |
|
dc.contributor.author |
Reddy, R.V. |
|
dc.contributor.author |
Nordlund, A. |
|
dc.date.accessioned |
2015-05-07T10:14:40Z |
|
dc.date.accessioned |
2021-02-12T09:34:56Z |
|
dc.date.available |
2015-05-07T10:14:40Z |
|
dc.date.available |
2021-02-12T09:34:56Z |
|
dc.date.issued |
1997 |
|
dc.identifier.citation |
Advances in Space Research, v.19/12, pp. 1785-1788, 1997. |
en_US |
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/54 |
|
dc.description.abstract |
2D reconnection is possible only in connection with the existence of a singularity in the magnetic field line topology, associated with a magnetic null point or a current sheet. Both of these provide an X-type structure of the magnetic field where fields of opposite polarity meet and reconnect. In 3D a similar topology is found in a null point pair, when the null points are connected by a separator line. The separator is defined as the intersection line of the two null-point fan planes. This paper reports on the topological evolution of this configuration with respect to different perturbations emerging from imposed boundary velocities, using a nonlinear numerical approach. |
en_US |
dc.language.iso |
en |
en_US |
dc.subject |
Magnetic reconnection |
en_US |
dc.subject |
Topology |
en_US |
dc.title |
Double null points and magnetic reconnection |
en_US |
dc.type |
Article |
en_US |
dc.identifier.accession |
090542 |
|