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Surface adjustment of the IRAM 30 m radio telescope
Authors:Morris  D Bremer  M Butin  G Carter  M Greve  A Lamb  JW Lazareff  B Lopez-Perez  J Mattiocco  F Penalver  J Thum  C
Affiliation:Institut de Radioastronomie Millimetrique (IRAM), 300 Rue de la Piscine, 38406 St Martin d?Heres, France E-mail: morris@iram.fr;
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 mm 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.
Keywords:
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