Radio emission regions in pulsars

Details Radio emission regions in pulsars Radio emission regions in pulsars

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.299..855k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 299, Issue 3, pp. 855-861.

Astronomy and Astrophysics

Astronomy

57

Stars: Atmospheres, Stars: Neutron, Pulsars: General

Scientific paper

We study the concept of radius-to-frequency mapping using a geometrical method for the estimation of pulsar emission altitudes. The semi-empirical relationship proposed by Kijak & Gil is examined over three decades of radio frequency. It is argued that the emission region in a millisecond pulsar occupies the magnetosphere over a distance of up to about 30 per cent of the light-cylinder radius, and that in a normal pulsar occupies up to approximately 10 per cent of the light-cylinder radius.

Affiliated with

Also associated with

No associations

Rating

Radio emission regions in 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 Radio emission regions in pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio emission regions in pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1711826