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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Cornwell, T.J. Golap, K. Bhatnagar, S. |
| Copyright Year | 2005 |
| Description | Author affiliation: Nat. Radio Astron. Obs., Socorro, NM, USA (Cornwell, T.J.; Golap, K.; Bhatnagar, S.) |
| Abstract | The new generation of synthesis radio telescopes now being proposed, designed, and constructed face substantial problems in making images over wide fields of view. Such observations are required either to achieve the full sensitivity limit in crowded fields or for surveys. The Square Kilometre Array (SKA Consortium, Tech. Rep., 2004), now being developed by an international consortium of 15 countries, will require advances well beyond the current state of the art. We review the theory of synthesis radio telescopes for large fields of view. We describe a new algorithm, W projection, for correcting the non-coplanar baselines aberration. This algorithm has improved performance over those previously used (typically an order of magnitude in speed). Despite the advent of W projection, the computing hardware required for SKA wide field imaging is estimated to cost up to $500M (2015 dollars). This is about half the target cost of the SKA. Reconfigurable computing is one way in which the costs can be decreased dramatically. |
| Sponsorship | IEEE Signal Processing Soc |
| File Size | 434474 |
| File Format | |
| ISBN | 0780388747 |
| ISSN | 15206149 |
| DOI | 10.1109/ICASSP.2005.1416440 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 2005-03-23 |
| Publisher Place | USA |
| Access Restriction | Subscribed |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Radio astronomy Costs Optical distortion Observatories Phased arrays RF signals Virtual manufacturing Equations Fourier transforms Optical interferometry |
| Content Type | Text |
| Resource Type | Article |
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