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Optimisation of the instrumental performance of IRMA

The Infrared Radiometer for Millimetre Astronomy (IRMA) is a passive atmospheric
water vapour monitor developed at the University of Lethbridge. It is a compact,
robust, and autonomous instrument, which is capable of being operated remotely. The
latest model is based on a PC/104 running an AMD 133 MHz SC520 processor, which
allows for more flexible control of the unit. The modifications and upgrades to the software required for the transition to this new platform are discussed in this thesis. In addition to software optimisation, a new calibration method has been developed as the unit has become better understood. This method has been verified through test campaigns carried out in Lethbridge and Chile. The results of these tests are included in this thesis. / xii, 141 leaves : ill. (some col.) ; 28 cm. --

Identiferoai:union.ndltd.org:LACETR/oai:collectionscanada.gc.ca:ALU.w.uleth.ca/dspace#10133/682
Date January 2008
CreatorsDahl, Regan Eugene, University of Lethbridge. Faculty of Arts and Science
ContributorsNaylor, David
PublisherLethbridge, Alta. : University of Lethbridge, Faculty of Arts and Science, 2008, Arts and Science, Department of Physics
Source SetsLibrary and Archives Canada ETDs Repository / Centre d'archives des thèses électroniques de Bibliothèque et Archives Canada
Languageen_US
Detected LanguageEnglish
TypeThesis
RelationThesis (University of Lethbridge. Faculty of Arts and Science)

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