Three-Dimensional Tomography of Pulsar Magnetospheres
Pulsars (rapidly spinning neutron stars) emit beams of intense radiation in the radio part of the electromagnetic spectrum. How these beams are generated remains one of the unsolved mysteries in astrophysics. By studying the pulse-to-pulse variations in their radiation using multiple telescopes simu...
| Main Author: | |
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| Format: | Thesis |
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Curtin University
2019
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| Online Access: | http://hdl.handle.net/20.500.11937/77427 |
| _version_ | 1848763847839580160 |
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| author | McSweeney, Samuel James |
| author_facet | McSweeney, Samuel James |
| author_sort | McSweeney, Samuel James |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | Pulsars (rapidly spinning neutron stars) emit beams of intense radiation in the radio part of the electromagnetic spectrum. How these beams are generated remains one of the unsolved mysteries in astrophysics. By studying the pulse-to-pulse variations in their radiation using multiple telescopes simultaneously, we can piece together a three-dimensional map of the intense environment surrounding these compact objects. The quasi-stable structures we observe in their radiation contain important clues to how the emission is generated. |
| first_indexed | 2025-11-14T11:09:58Z |
| format | Thesis |
| id | curtin-20.500.11937-77427 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T11:09:58Z |
| publishDate | 2019 |
| publisher | Curtin University |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-774272019-12-18T02:54:40Z Three-Dimensional Tomography of Pulsar Magnetospheres McSweeney, Samuel James Pulsars (rapidly spinning neutron stars) emit beams of intense radiation in the radio part of the electromagnetic spectrum. How these beams are generated remains one of the unsolved mysteries in astrophysics. By studying the pulse-to-pulse variations in their radiation using multiple telescopes simultaneously, we can piece together a three-dimensional map of the intense environment surrounding these compact objects. The quasi-stable structures we observe in their radiation contain important clues to how the emission is generated. 2019 Thesis http://hdl.handle.net/20.500.11937/77427 Curtin University fulltext |
| spellingShingle | McSweeney, Samuel James Three-Dimensional Tomography of Pulsar Magnetospheres |
| title | Three-Dimensional Tomography of Pulsar Magnetospheres |
| title_full | Three-Dimensional Tomography of Pulsar Magnetospheres |
| title_fullStr | Three-Dimensional Tomography of Pulsar Magnetospheres |
| title_full_unstemmed | Three-Dimensional Tomography of Pulsar Magnetospheres |
| title_short | Three-Dimensional Tomography of Pulsar Magnetospheres |
| title_sort | three-dimensional tomography of pulsar magnetospheres |
| url | http://hdl.handle.net/20.500.11937/77427 |