Models for axially symmetric pulsar magnetospheres

Details Models for axially symmetric pulsar magnetospheres Models for axially symmetric pulsar magnetospheres

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cpp..conf...98n&link_type=abstract

In Max-Planck-Inst. für Physik und Astrophysik, Cosmic Plasma Physics p 98-102 (SEE N89-25716 19-75)

Physics

Plasma Physics

Cosmic Plasma, Magnetospheres, Particle Density (Concentration), Pulsars, Magnetic Field Configurations, Magnetospheric Electron Density, Plasma Control, Stellar Magnetic Fields

Scientific paper

A method for the construction of self-consistent models for an axially symmetric pulsar magnetosphere (parallel rotator) neglecting radiation effects is presented. Results obtained for nonrelativistic magnetospheres are shown. For the quasi-neutral case, starting from a vacuum dipole field the particle density is increased. A dipole field can only store a limited amount of plasma. For the neutral case, the electric potential changes considerably, whereas the magnetic field remains nearly unchanged.

Affiliated with

Also associated with

No associations

Rating

Models for axially symmetric pulsar magnetospheres does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Models for axially symmetric pulsar magnetospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Models for axially symmetric pulsar magnetospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1825852