Dish Surface Accuracy
Dish Surface Accuracy is a metrological metric that quantifies the deviation of a radio telescope's reflector surface from its ideal geometric shape, typically expressed as a root-mean-square error, to ensure optimal electromagnetic wave focusing and minimize signal loss.
9
Publications
325
Citations
75
Authors
10
Institutions
Publications per year
2017–2026
0
Parents
9
1–5 of 9
75
2
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10
California Institute of Technology
Pasadena, United States
2 h-index
3 publications
90 citations

Caltech Submillimeter Observatory
Hilo, United States
1 h-index
5 publications
100 citations
University of Cambridge
Cambridge, United Kingdom
1 h-index
2 publications
214 citations

Search for Extraterrestrial Intelligence
Mountain View, United States
1 h-index
17 publications
527 citations
Freie Universität Berlin
Berlin, Germany
1 h-index
1 publications
32 citations
University of California, Berkeley
Berkeley, United States
1 h-index
30 publications
930 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
1 h-index
1 publications
35 citations
University of Monastir
Monastir, Tunisia
1 h-index
1 publications
29 citations
1–8 of 10
2 publications · 35 citations
2
h-index
1 publications · 32 citations
1
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1 publications · 29 citations
1
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1 publications · 40 citations
1
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1 publications · 107 citations
1
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