Pulsar Magnetic Field Oscillation Model and Verification Method

Details Pulsar Magnetic Field Oscillation Model and Verification Method Pulsar Magnetic Field Oscillation Model and Verification Method

2007-09-27

arxiv.org/abs/0709.4315v1

Astronomy and Astrophysics

Astrophysics

21 pages, 4 figures

Scientific paper

We constructed the magnetic field oscillation model (hereafter the MO model) by analogizing the periodically reversing phenomenon of the solar magnetic field to pulsars. Almost all kinds of pulsar radiation phenomena are best explained using the MO model, especially polarization characteristics, glitch, generation rate, the geodetic precession of pulsars and the configuration of pulsar-wind nebula of the Crab. The MO model also provides a satisfactory explanation of other characteristics of pulsars, e.g., interpulse, spin-down, pulse nulling, beat and pulse drift, the loss rate of the rotating energy, and the accuracy of frequency. We present six verification methods for the MO model. In addition, we predict that the pulsar PSR B1913+16 will not disappear from our line of sight after the year 2025, which is antithetical to the prediction made by some astronomers.

Affiliated with

Also associated with

No associations

Rating

Pulsar Magnetic Field Oscillation Model and Verification Method 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 Pulsar Magnetic Field Oscillation Model and Verification Method, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsar Magnetic Field Oscillation Model and Verification Method will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-481190