The pulsar radio emission originates from regions below 10% of the light cylinder radius.
This requires a mechanism where coherent emission is excited in relativistic pair plasma …

The diverse polarization properties in pulsars are in conflict with applying a unique emission
mechanism to the population. The polarization position angle (PPA) traverse in most pulsars …

A detailed analysis of nulling was conducted for the pulsars studied in the Meterwavelength
Single-pulse Polarimetric Emission Survey. We characterized nulling in 36 pulsars including …

We present radio pulsar emission beam analyses and models with the primary intent of
examining pulsar beam geometry and physics over the broadest band of radio frequencies …

The S-shaped swing of the linear polarization position angle (PPA) observed in many
pulsars can be interpreted by the rotating vector model (RVM). However, efforts to fit the …

We report on an Arecibo 4.5-GHz polarimetric single-pulse survey of the brightest pulsars at
high frequency within its sky. The high-frequency profiles are accompanied by a collection of …

We present integrated pulse profiles at 5 GHz for 71 pulsars, including eight millisecond
pulsars (MSPs), obtained using the Shanghai Tian Ma Radio Telescope. Mean flux densities …

ABSTRACT A potential resolution for the generation of coherent radio emission in pulsar
plasma is the existence of relativistic charge solitons, which are solutions of non-linear …

The core component width in normal pulsars, with periods (P)> 0.1 s, measured at the half-
power point at 1 GHz, has a lower boundary line (LBL) that closely follows the P− 0.5 scaling …

In this paper, we study a set of 12 pulsars that previously had not been characterized. Our
timing shows that eleven of them are 'normal'isolated pulsars, with rotation periods between …