Interstellar scattering - New diagnostics of pulsars and the ISM
Extreme Scattering Events and pulsar secondary spectra have highlighted fundamental problems in our understanding of the dynamics of interstellar turbulence. We describe some of these problems in detail and present the theory behind the technique of speckle imaging, which offers a prospect of reveal...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Conference Paper |
| Published: |
International Astronomical Union
2013
|
| Subjects: | |
| Online Access: | http://hdl.handle.net/20.500.11937/21428 |
| _version_ | 1848750587639758848 |
|---|---|
| author | Macquart, Jean-Pierre |
| author2 | J. van Leeuwen |
| author_facet | J. van Leeuwen Macquart, Jean-Pierre |
| author_sort | Macquart, Jean-Pierre |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | Extreme Scattering Events and pulsar secondary spectra have highlighted fundamental problems in our understanding of the dynamics of interstellar turbulence. We describe some of these problems in detail and present the theory behind the technique of speckle imaging, which offers a prospect of revealing fundamental properties of the turbulence. It also offers the prospect of resolving pulsar magnetospheres on ~ 10 nas scales. |
| first_indexed | 2025-11-14T07:39:12Z |
| format | Conference Paper |
| id | curtin-20.500.11937-21428 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T07:39:12Z |
| publishDate | 2013 |
| publisher | International Astronomical Union |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-214282017-09-13T13:54:25Z Interstellar scattering - New diagnostics of pulsars and the ISM Macquart, Jean-Pierre J. van Leeuwen ISM: structure ISM: magnetic fields scattering turbulence Extreme Scattering Events and pulsar secondary spectra have highlighted fundamental problems in our understanding of the dynamics of interstellar turbulence. We describe some of these problems in detail and present the theory behind the technique of speckle imaging, which offers a prospect of revealing fundamental properties of the turbulence. It also offers the prospect of resolving pulsar magnetospheres on ~ 10 nas scales. 2013 Conference Paper http://hdl.handle.net/20.500.11937/21428 10.1017/S1743921312023708 International Astronomical Union fulltext |
| spellingShingle | ISM: structure ISM: magnetic fields scattering turbulence Macquart, Jean-Pierre Interstellar scattering - New diagnostics of pulsars and the ISM |
| title | Interstellar scattering - New diagnostics of pulsars and the ISM |
| title_full | Interstellar scattering - New diagnostics of pulsars and the ISM |
| title_fullStr | Interstellar scattering - New diagnostics of pulsars and the ISM |
| title_full_unstemmed | Interstellar scattering - New diagnostics of pulsars and the ISM |
| title_short | Interstellar scattering - New diagnostics of pulsars and the ISM |
| title_sort | interstellar scattering - new diagnostics of pulsars and the ism |
| topic | ISM: structure ISM: magnetic fields scattering turbulence |
| url | http://hdl.handle.net/20.500.11937/21428 |