Abstract
In aperture synthesis measurements in Radioastronomy, the measurement set is frequently three-dimensional (in space) and therefore cannot be simply represented in two-dimensions. As a result, the point spread function for the instrument varies as a function of direction. This has been considered in recent publications in relation to digital data processing and some of the features of the three-dimensional problem, and methods for implementing the computation using one or two-dimensional transforms will be presented.
Original language | English |
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Title of host publication | SPIE Proceedings 0231 |
Subtitle of host publication | 1980 International Optical Computing Conference 1 |
Editors | William T. Rhodes |
Place of Publication | Bellingham, Washington |
Pages | 26-29 |
Number of pages | 4 |
Volume | 231 |
DOIs | |
Publication status | Published - 22 Aug 1980 |
Externally published | Yes |
Event | 1980 International Optical Computing Conference I - Washington, United States Duration: 8 Apr 1980 → 8 Apr 1980 |
Conference
Conference | 1980 International Optical Computing Conference I |
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Country | United States |
City | Washington |
Period | 8/04/80 → 8/04/80 |