Add to ORKGPolarization is one of the striking characteristies of pulsar's emission. The integrated profiles of a number of pulsars have intensive linear polarization. The position angle of the linearly polarized emission varies throughout the profile. For most pulsars this variation is continuous and ofte...121597-160
Pulsar radio emission is generally found to be linearly polarized over all longitudes of profiles, s...
We report on polarimetric observations of 100 pulsars centered on 774 MHz, made using the Green Bank...
We present strong observational evidence for a relationship between the direction of a pulsar's moti...
One of the most important properties of radio emission of pulsars is the high linear polarization. M...
The linear polarization position angle (PPA) of pulsar emission shows a wide variety of structures, ...
We present here a direct comparison of the polarization position angle (PA) profiles of 17 pulsars, ...
We present a systematic study of the circular polarization in pulsar integrated profiles, based on p...
The circular polarization associated with pulsar emission is examined phenomenologically. Virtually ...
The observed polarisation angle variation in pulsars is analysed on the basis of the magnetic pole m...
Abstract. Pulsar Β1929+10 is remarkable on a number of grounds. Its narrow primary components exhibi...
We present here a direct comparison of the polarisation position angle (PA) profiles of 17 pulsars, ...
Polarization observations of the radio emission from PSR B2016+28 at 1404 MHz reveal properties that...
Polarization profiles are presented for 20 millisecond pulsars that are being observed as part of th...
We suggest that the observed linear polarization of pulsar radio emission is due to features of the ...
We use a set of carefully selected published average multifrequency polarimetric observations for si...
Pulsar radio emission is generally found to be linearly polarized over all longitudes of profiles, s...
We report on polarimetric observations of 100 pulsars centered on 774 MHz, made using the Green Bank...
We present strong observational evidence for a relationship between the direction of a pulsar's moti...
One of the most important properties of radio emission of pulsars is the high linear polarization. M...
The linear polarization position angle (PPA) of pulsar emission shows a wide variety of structures, ...
We present here a direct comparison of the polarization position angle (PA) profiles of 17 pulsars, ...
We present a systematic study of the circular polarization in pulsar integrated profiles, based on p...
The circular polarization associated with pulsar emission is examined phenomenologically. Virtually ...
The observed polarisation angle variation in pulsars is analysed on the basis of the magnetic pole m...
Abstract. Pulsar Β1929+10 is remarkable on a number of grounds. Its narrow primary components exhibi...
We present here a direct comparison of the polarisation position angle (PA) profiles of 17 pulsars, ...
Polarization observations of the radio emission from PSR B2016+28 at 1404 MHz reveal properties that...
Polarization profiles are presented for 20 millisecond pulsars that are being observed as part of th...
We suggest that the observed linear polarization of pulsar radio emission is due to features of the ...
We use a set of carefully selected published average multifrequency polarimetric observations for si...
Pulsar radio emission is generally found to be linearly polarized over all longitudes of profiles, s...
We report on polarimetric observations of 100 pulsars centered on 774 MHz, made using the Green Bank...
We present strong observational evidence for a relationship between the direction of a pulsar's moti...