HXHongwei Xu
Hongwei Xu
*This is an algorithmically generated author record based on publicly available information.
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
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Research Interests
Hongwei Xu has a total of 12 co-authors. Here are the top co-authors by number of shared publications:
- Hui Liu
School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550025, China
1 shared publication - Lun-Hua Shang
Guizhou Normal University
1 shared publication - Qi-Jun Zhi
Guizhou Normal University
1 shared publication - Ru-Shuang Zhao
Guizhou Normal University
1 shared publication - Ruwen Tian
School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550025, China
1 shared publication - Shidong Wang
School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550025, China
1 shared publication
Latest Publications
- Open Access
Statistical Study on the Q Parameter Based on Parkes Data
Using the rotating vector model (RVM) and aiming to constrain the value of the magnetic inclination angle (), we perform a least-squares fit on the linearly polarized position angles of 125 pulsars from Parkes 64 m archive data at 1400 MHz. Subsequently, a statistical analysis of the normalized Q parameters is carried out. Furthermore, based on the Q-parameter, we provide a further understanding of the geometry of the radio emission region of the pulsar. In this statistical sample, about 1/5 of the sample is clustered at 0, suggesting that this part of the pulsar is viewed from the center of the radiation cone. For the rest of the pulsars, the Q parameters follow a uniform distribution, supporting the conclusion that the interface of the radiation cone is non-elliptical.Open AccessStatistical Study on the Q Parameter Based on Parkes Data
Using the rotating vector model (RVM) and aiming to constrain the value of the magnetic inclination angle (), we perform a least-squares fit on the linearly polarized position angles of 125 pulsars from Parkes 64 m archive data at 1400 MHz. Subsequently, a statistical analysis of the normalized Q parameters is carried out. Furthermore, based on the Q-parameter, we provide a further understanding of the geometry of the radio emission region of the pulsar. In this statistical sample, about 1/5 of the sample is clustered at 0, suggesting that this part of the pulsar is viewed from the center of the radiation cone. For the rest of the pulsars, the Q parameters follow a uniform distribution, supporting the conclusion that the interface of the radiation cone is non-elliptical.