Radio pulsars - Intensity, polarization, and rotation fluctuations

Details Radio pulsars - Intensity, polarization, and rotation fluctuations Radio pulsars - Intensity, polarization, and rotation fluctuations

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aipc..101...98c&link_type=abstract

IN: Positron-electron pairs in astrophysics; Proceedings of the Workshop, Greenbelt, MD, January 6-8, 1983 (A85-31276 13-90). Ne

Astronomy and Astrophysics

Astrophysics

10

Pulsar Magnetospheres, Pulsars, Radio Stars, Stellar Radiation, Polarized Electromagnetic Radiation, Radio Emission, Stellar Evolution, Stellar Rotation, Waveforms

Scientific paper

In this review of radio emission phenomena emphasis is given to observables that may constrain the particle content in pulsar magnetospheres. These include intensity variations within single pulses (time scales from 1 microsec to tens of milliseconds); pulse-to-pulse variations (one period to years) which are both 'continuous' (drifts of subpulse features through pulse phase and other quasiperiodic and aperiodic variations) and discontinuous' (pulse nulling, average pulse shape changes, changes in drift rates); polarization transitions between orthogonal models; relationship of drifting subpulses to nulling; constraints on emission altitudes; and rotation noise due to internal and magnetospheric torque fluctuations.

Affiliated with

Also associated with

No associations

Rating

Radio pulsars - Intensity, polarization, and rotation fluctuations 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 pulsars - Intensity, polarization, and rotation fluctuations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio pulsars - Intensity, polarization, and rotation fluctuations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1626629