Please use this identifier to cite or link to this item:
http://arks.princeton.edu/ark:/88435/dsp01k930bx153
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor | Li, Jason | - |
dc.contributor.other | NASA | en_US |
dc.creator | Li, Jason | - |
dc.creator | Spitkovsky, Anatoly | - |
dc.date.accessioned | 2013-11-21T19:55:51Z | - |
dc.date.available | 2013-11-21T19:55:51Z | - |
dc.date.issued | 2013-11-21 | - |
dc.identifier.uri | http://arks.princeton.edu/ark:/88435/dsp01k930bx153 | - |
dc.description.abstract | Magnetic field lines and current sheets for an orbiting neutron star binary with the magnetic moments of both stars aligned with the rotation axis. The stars are not spinning, i.e., R_{LC,∗} = ∞. Fields are by and large confined to the half of the magnetosphere closer to their source star. This movie shows the corotating field pattern as the orbit progresses. | en_US |
dc.language.iso | en_US | en_US |
dc.subject | neutron stars | en_US |
dc.title | Aligned Nonspinning Dipoles | en_US |
dc.type | moving image | en_US |
pu.projectgrantnumber | 120-6425 | en_US |
Appears in Collections: | Research Data Sets |
Files in This Item:
File | Description | Size | Format | |
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t0sinf.mpeg | 13.88 MB | MPEG | View/Download |
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