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DC Field | Value | Language |
---|---|---|
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 | |
Appears in Collections: | UAS_Reprints |
Files in This Item:
File | Description | Size | Format | |
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ReddyRV_etal_AdvSpRes_1997.pdf Restricted Access | 358.81 kB | Adobe PDF | View/Open Request a copy |
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