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dc.contributor.authorMacquart, Jean-Pierre
dc.contributor.editorJ. van Leeuwen
dc.date.accessioned2017-01-30T12:25:05Z
dc.date.available2017-01-30T12:25:05Z
dc.date.created2014-02-27T20:00:42Z
dc.date.issued2013
dc.identifier.citationMacquart, Jean-Pierre. 2013. Interstellar scattering - New diagnostics of pulsars and the ISM, in van Leeuwen, J. (ed), Proceedings of the International Astronomical Union Symposium S291, Aug 20-31 2012, 8: pp. 217-222. Beijing, China: International Astronomical Union.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/21428
dc.identifier.doi10.1017/S1743921312023708
dc.description.abstract

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.

dc.publisherInternational Astronomical Union
dc.subjectISM: structure
dc.subjectISM: magnetic fields
dc.subjectscattering
dc.subjectturbulence
dc.titleInterstellar scattering - New diagnostics of pulsars and the ISM
dc.typeConference Paper
dcterms.source.startPage217
dcterms.source.endPage222
dcterms.source.titleNeutron Stars and Pulsars: Challenges and Opportunities after 80 years
dcterms.source.seriesNeutron Stars and Pulsars: Challenges and Opportunities after 80 years
dcterms.source.conferenceProceedings of the International Astronomical Union
dcterms.source.conference-start-dateAug 20 2012
dcterms.source.conferencelocationBeijing, China
dcterms.source.placeFrance
curtin.note

Copyright © 2013 Cambridge University Press

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curtin.accessStatusOpen access


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