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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3757
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dc.contributor.authorMorris, D.-
dc.contributor.authorBremer, M.-
dc.contributor.authorButin, G.-
dc.contributor.authorCarter, M.-
dc.contributor.authorGreve, A.-
dc.contributor.authorLamb, J.W.-
dc.contributor.authorLazareff, B.-
dc.contributor.authorLopez-Perez, J.-
dc.contributor.authorMattiocco, F.-
dc.contributor.authorPenalver, J.-
dc.contributor.authorThum, C.-
dc.date.accessioned2009-05-18T06:39:01Z-
dc.date.available2009-05-18T06:39:01Z-
dc.date.issued2009-01-23-
dc.identifier.citationIET Microwaves, Antennas & Propagation, 2009, Vol. 3(1), p99-108en
dc.identifier.issn1751-8725-
dc.identifier.issn1751-8733 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/3757-
dc.descriptionRestricted Access.en
dc.description.abstractThe 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.isoenen
dc.publisherInstitution of Engineering and Technologyen
dc.relation.urihttp://dx.doi.org/10.1049/iet-map:20080044en
dc.rights2009 Institution of Engineering and Technologyen
dc.titleSurface adjustment of the IRAM 30 m radio telescopeen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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