Drift Wave Model of Part Time Radio Pulsars

Details Drift Wave Model of Part Time Radio Pulsars Drift Wave Model of Part Time Radio Pulsars

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..983..100l&link_type=abstract

40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP Conference Proceedings, Volume 983, pp. 100-102 (2008).

Physics

Pulsars, Neutron Stars, Magnetohydrodynamics And Plasmas, Radiation Mechanisms, Polarization

Scientific paper

During the last few years there were discovered and deeply examined several transient neutron stars (Part Time Radio Pulsars). It is already well accepted that these objects are rotating neutron stars. But their extraordinary features (burst-like behavior) made necessary revision of well accepted models of pulsar interior structure. Nowadays most popular model for part time radio pulsars is precessing pulsar model, which is the subject of big discussion. We assume that these objects are pulsars with specific spin parameters. An important feature of our model, naturally explaining most of the properties of these neutron stars, is presence of very low frequency, nearly transverse drift waves propagating across the magnetic field and encircling the open field lines region of the pulsar magnetosphere.

Affiliated with

Also associated with

No associations

Rating

Drift Wave Model of Part Time Radio Pulsars 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 Drift Wave Model of Part Time Radio Pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Drift Wave Model of Part Time Radio Pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1872897