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http://hdl.handle.net/2289/3757
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DC Field | Value | Language |
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dc.contributor.author | Morris, D. | - |
dc.contributor.author | Bremer, M. | - |
dc.contributor.author | Butin, G. | - |
dc.contributor.author | Carter, M. | - |
dc.contributor.author | Greve, A. | - |
dc.contributor.author | Lamb, J.W. | - |
dc.contributor.author | Lazareff, B. | - |
dc.contributor.author | Lopez-Perez, J. | - |
dc.contributor.author | Mattiocco, F. | - |
dc.contributor.author | Penalver, J. | - |
dc.contributor.author | Thum, C. | - |
dc.date.accessioned | 2009-05-18T06:39:01Z | - |
dc.date.available | 2009-05-18T06:39:01Z | - |
dc.date.issued | 2009-01-23 | - |
dc.identifier.citation | IET Microwaves, Antennas & Propagation, 2009, Vol. 3(1), p99-108 | en |
dc.identifier.issn | 1751-8725 | - |
dc.identifier.issn | 1751-8733 (Online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/3757 | - |
dc.description | Restricted Access. | en |
dc.description.abstract | The techniques used to set and stabilise the surface of the IRAM 30 m radio telescope to a final root mean square accuracy of about 50 µm are described. This involved both phase retrieval and phase coherent holography using a variety of radiation sources at several frequencies. A finite-element model was utilised in improving the temperature control system for the telescope structure. The factors influencing the ultimate surface accuracy are discussed. | en |
dc.language.iso | en | en |
dc.publisher | Institution of Engineering and Technology | en |
dc.relation.uri | http://dx.doi.org/10.1049/iet-map:20080044 | en |
dc.rights | 2009 Institution of Engineering and Technology | en |
dc.title | Surface adjustment of the IRAM 30 m radio telescope | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2009 IET_MAP V3 p99-108.pdf Restricted Access | 10p. | 509.24 kB | Adobe PDF | View/Open Request a copy |
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