Radiation Properties of Pulsar Magnetospheres: Observation, Theory, and Experiment

Details Radiation Properties of Pulsar Magnetospheres: Observation, Theory, and Experiment Radiation Properties of Pulsar Magnetospheres: Observation, Theory, and Experiment

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.227..229h&link_type=abstract

Astrophysics and Space Science, Volume 227, Issue 1-2, pp. 229-253

Astronomy and Astrophysics

Astrophysics

1

Pulsars, Radio Astronomy, Plasma Astrophysics

Scientific paper

In the three decades since their discovery, the accumulated body of observational data from pulsar sources puts constraints on models that seek to explain their periodic radiation. This paper reviews this data, reports on a VLA search for haloes predicted by an early model, and reinvestigates a magnetospheric disk-field-aligned-current transmission line system as the origin of the observed radiation, with external wave excitation by as yet an unexplained source. Three dimensional, fully electromagnetic particle-in-cell simulations of the pulsar surface and magnetosphere are used to explore the waveshape and polarization properties of the observed radiation.

Affiliated with

Also associated with

No associations

Rating

Radiation Properties of Pulsar Magnetospheres: Observation, Theory, and Experiment 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 Radiation Properties of Pulsar Magnetospheres: Observation, Theory, and Experiment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation Properties of Pulsar Magnetospheres: Observation, Theory, and Experiment will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1058270