Paper
28 September 2004 Initial results of field testing an infrared water vapor monitor for millimeter astronomy (IRMA III) on Mauna Kea
Robin R. Phillips, David A. Naylor, James diFrancesco, Brad Gom
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Abstract
The Infrared Radiometer for Millimetre wavelength Astronomy (IRMA) is a compact, light weight, low cost, low maintainance water vapour monitor, with an accuracy that enables it to be used to correct the phase distortions caused by atmospheric water vapour in millimetre wavelength interferometers. The IRMA III prototype is a major improvement on earlier versions of IRMA, with an emphasis on simplicity and reliability. We present results of tests conducted on the Smithsonian Millimeter Array (SMA) telescope on Mauna Kea in February 2004. The test campaign involved using three IRMA III devices with the SMA to provide phase correction information for improving the quality of the astronomical interferometric data.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Robin R. Phillips, David A. Naylor, James diFrancesco, and Brad Gom "Initial results of field testing an infrared water vapor monitor for millimeter astronomy (IRMA III) on Mauna Kea", Proc. SPIE 5489, Ground-based Telescopes, (28 September 2004); https://doi.org/10.1117/12.548458
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Cited by 4 scholarly publications.
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KEYWORDS
Shape memory alloys

Astronomy

Telescopes

Antennas

Infrared astronomy

Infrared radiation

Connectors

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