Tackling radio polarization data of high energy pulsars

Placeholder Show Content

Abstract/Contents

Abstract
The focus of this thesis is on understanding the pulsar magnetosphere particularly with the exploitation of radio polarization. The rotating vector model (the standard pulsar polarization model) can be modified to estimate emission altitude. However, more realistic treatment of relativistic and sweep-back effects show that such augmentations break down relatively quickly. This break-down is quantified and fitting functions are provided that preserve accuracy to higher altitude. The rotating vector model has proven particularly poor for modeling energetic pulsars. We remedy this by including the effects of orthogonal mode jumps, multiple emission altitudes, open zone growth via y-point lowering, and interstellar scattering. A large number of discrepancies can be understood while retaining the geometric picture. The model is systematically applied to six Fermi-detected pulsars (PSR J0023+0923, PSR J1024−0719, PSR J1744−1134, PSR J1057−5226, PSR J1420−6048, and PSR J2124−3358). Several other examples of utilizing polarization modeling to understand pulsar geometry and emission characteristics are also presented. Finally, a bidirectional emission model is applied to the polarization data of PSR J1057−5226 and PSR J1705−1906. Overall, we push the limit of what can be learned from a geometrically based model and emphasize the importance of tying such models to data.

Description

Type of resource text
Form electronic; electronic resource; remote
Extent 1 online resource.
Publication date 2015
Issuance monographic
Language English

Creators/Contributors

Associated with Craig, Helen Alta
Associated with Stanford University, Department of Applied Physics.
Primary advisor Bucksbaum, Philip H
Primary advisor Romani, Roger W. (Roger William)
Thesis advisor Bucksbaum, Philip H
Thesis advisor Romani, Roger W. (Roger William)
Thesis advisor Blandford, Roger D
Advisor Blandford, Roger D

Subjects

Genre Theses

Bibliographic information

Statement of responsibility Helen Alta Craig.
Note Submitted to the Department of Applied Physics.
Thesis Thesis (Ph.D.)--Stanford University, 2015.
Location electronic resource

Access conditions

Copyright
© 2015 by Helen Craig
License
This work is licensed under a Creative Commons Attribution Non Commercial 3.0 Unported license (CC BY-NC).

Also listed in

Loading usage metrics...