Pulsar Interstellar Scattering
Pulsar Interstellar Scattering is a physical phenomenon in pulsar astronomy characterized by the distortion of pulsed radio emission due to multipath propagation caused by density inhomogeneities in the interstellar medium, leading to temporal broadening and intensity fluctuations of the observed signal.
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10.6K
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545
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210
Institutions
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2017–2026
38
Variants
Interstellar Scattering Of Pulsars
Parents
183
FAST RADIO BURST DISCOVERED IN THE ARECIBO PULSAR ALFA SURVEY
L. G. Spitler, J. M. Cordes, J. W. T. Hessels et al. · The Astrophysical Journal · 2014 · 519 citations · Full text
Natural Sciences, Astronomy, Physics +13
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University of Manchester
Manchester, United Kingdom
25 h-index
75 publications
3.9K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
22 h-index
107 publications
5.9K citations
National Radio Astronomy Observatory
Charlottesville, United States
21 h-index
52 publications
2.5K citations

Cornell University
Ithaca, United States
19 h-index
46 publications
5.2K citations
Netherlands Institute for Radio Astronomy
Dwingeloo, The Netherlands
18 h-index
59 publications
4.7K citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
18 h-index
43 publications
2.3K citations
Swinburne University of Technology
Melbourne, Australia
17 h-index
21 publications
976 citations
Oberlin College
Oberlin, United States
15 h-index
38 publications
2.7K citations
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ApJ · 73 publications · 5.9K citations
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4 publications · 207 citations
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