Interstellar Scintillation is a radiative propagation phenomenon in which the observed intensity and phase of electromagnetic waves from compact astrophysical sources vary over time due to refractive and diffractive effects caused by electron density fluctuations in the turbulent interstellar medium.
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2017–2026
45
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288
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807
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22
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294
National Radio Astronomy Observatory
Charlottesville, United States
26 h-index
60 publications
3.6K citations
Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
26 h-index
144 publications
9.1K citations
Australia Telescope National Facility
Sydney, Australia
25 h-index
107 publications
8.5K citations
University of California San Diego
San Diego, United States
25 h-index
49 publications
2.7K citations
Cornell University
Ithaca, United States
23 h-index
53 publications
4.2K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
23 h-index
123 publications
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University of Manchester
Manchester, United Kingdom
22 h-index
68 publications
4.3K citations
The University of Sydney
Sydney, Australia
21 h-index
53 publications
3.3K citations
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ApJ · 106 publications · 8.1K citations
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19 publications · 486 citations
15
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Repository · 7 publications · 343 citations
7
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- The Astrophysical Journal Letters
6 publications · 282 citations
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