Aligned Rapidly Spinning Dipoles

Li, Jason
Issue date: 2013
Rights:
 Creative Commons Attribution 4.0 International (CC BY)
Cite as:
Li, Jason. (2013). Aligned Rapidly Spinning Dipoles [Data set]. Princeton University. https://doi.org/10.34770/er0g-mk31
@electronic{li_jason_2013,
  author      = {Li, Jason},
  title       = {{Aligned Rapidly Spinning Dipoles}},
  publisher   = {{Princeton University}},
  year        = 2013,
  url         = {https://doi.org/10.34770/er0g-mk31}
}
Description:

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 spinning rapidly at ∼ ms periods, with R_{LC,∗}/R_∗ = 2.7. Stellar spin winds fields backwards toroidally, and they can propagate to the far side of the magnetosphere closer to the opposing star. This movie shows the corotating field pattern as the orbit progresses.

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More about this record
Author Li, Jason
Domains Natural Sciences
Communities Astrophysical Sciences
Issue date 2013
Date Created 2013-01-01
Date Modified 2024-08-07
URI https://doi.org/10.34770/er0g-mk31
URI http://arks.princeton.edu/ark:/88435/dsp019w032314c
Publisher Princeton University
Type Dataset
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