Differential Image Motion
Differential Image Motion is a metric in observational astronomy that quantifies the degradation of astronomical image quality due to atmospheric turbulence by measuring the differences in positional shifts of a star's image across two or more spatially separated subapertures of a telescope.
83
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3.8K
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338
Authors
121
Institutions
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2017–2026
14
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The ESO differential image motion monitor
M. Sarazin, F. Roddier · 1990 · 256 citations
Sidekick 2 directs formation of a retinal circuit that detects differential motion
Arjun Krishnaswamy, Masahito Yamagata, Xin Duan et al. · Nature · 2015 · 177 citations · Full text
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Université Côte d'Azur
Nice, France
10 h-index
33 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
49 publications
1.5K citations
European Southern Observatory
Garching bei München, Germany
7 h-index
27 publications
838 citations
Cerro Tololo Inter-American Observatory
La Serena, Chile
5 h-index
8 publications
588 citations
National Astronomical Observatories
Beijing, China
5 h-index
30 publications
638 citations

Chinese Academy of Sciences
Beijing, China
5 h-index
49 publications
1.1K citations

W.M. Keck Observatory
Waimea, United States
4 h-index
9 publications
240 citations
Observatoire de la Côte d’Azur
Nice, France
4 h-index
32 publications
878 citations
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PASP · 12 publications · 721 citations
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14 publications · 565 citations
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8 publications · 116 citations
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7 publications · 177 citations
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