Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer

We report calibration of the optical instruments of the Optical Mesosphere Thermosphere Imagers (OMTI) using facilities at the National Institute of Polar Research. OMTI has been developed to investigate dynamics of the upper atmosphere through nocturnal airglow emissions. OMTI consist of an imaging...

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Main Authors: Yasuo Katoh, Kazuo Shiokawa, Mitsugi Satoh, Mitsumu K. Ejiri, Tadahiko Ogawa
Format: Article
Language:English
Published: National Institute of Polar Research 1999-03-01
Series:Antarctic Record
Online Access:http://doi.org/10.15094/00009066
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spelling doaj-c1548565e68f4384aba53c4fab99602b2020-11-24T23:11:33ZengNational Institute of Polar ResearchAntarctic Record0085-72892432-079X1999-03-0143111510.15094/00009066Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometerYasuo Katoh0Kazuo Shiokawa1Mitsugi Satoh2Mitsumu K. Ejiri3Tadahiko Ogawa4 Solar-Terrestrial Environment Laboratory, Nagoya University Solar-Terrestrial Environment Laboratory, Nagoya University Solar-Terrestrial Environment Laboratory, Nagoya University Solar-Terrestrial Environment Laboratory, Nagoya University Solar-Terrestrial Environment Laboratory, Nagoya University We report calibration of the optical instruments of the Optical Mesosphere Thermosphere Imagers (OMTI) using facilities at the National Institute of Polar Research. OMTI has been developed to investigate dynamics of the upper atmosphere through nocturnal airglow emissions. OMTI consist of an imaging Fabry-Perot interferometer, three all-sky cooled-CCD cameras, three tilting-photometers, and a spectral airglow temperature imager (SATI). The all-sky cameras and the photometers have been calibrated using a 2-m integrating-sphere and a spectrometer. Absolute sensitivity and image-flattening data are obtained together with filter transmission functions. Inhomogeneity of transmission function on the filter surface is found from the calibration using the spectrometer. We also find that filters with highly-flattened image-quality surfaces may cause serious Newton's Ring pattern on final images. Examples of the data are shown for the cameras and the photometers based on the airglow observation at Shigaraki (35°N, 136°E), Japan.http://doi.org/10.15094/00009066
collection DOAJ
language English
format Article
sources DOAJ
author Yasuo Katoh
Kazuo Shiokawa
Mitsugi Satoh
Mitsumu K. Ejiri
Tadahiko Ogawa
spellingShingle Yasuo Katoh
Kazuo Shiokawa
Mitsugi Satoh
Mitsumu K. Ejiri
Tadahiko Ogawa
Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer
Antarctic Record
author_facet Yasuo Katoh
Kazuo Shiokawa
Mitsugi Satoh
Mitsumu K. Ejiri
Tadahiko Ogawa
author_sort Yasuo Katoh
title Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer
title_short Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer
title_full Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer
title_fullStr Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer
title_full_unstemmed Calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer
title_sort calibration of all-sky cameras and tilting-photometers using an integrating-sphere and a spectrometer
publisher National Institute of Polar Research
series Antarctic Record
issn 0085-7289
2432-079X
publishDate 1999-03-01
description We report calibration of the optical instruments of the Optical Mesosphere Thermosphere Imagers (OMTI) using facilities at the National Institute of Polar Research. OMTI has been developed to investigate dynamics of the upper atmosphere through nocturnal airglow emissions. OMTI consist of an imaging Fabry-Perot interferometer, three all-sky cooled-CCD cameras, three tilting-photometers, and a spectral airglow temperature imager (SATI). The all-sky cameras and the photometers have been calibrated using a 2-m integrating-sphere and a spectrometer. Absolute sensitivity and image-flattening data are obtained together with filter transmission functions. Inhomogeneity of transmission function on the filter surface is found from the calibration using the spectrometer. We also find that filters with highly-flattened image-quality surfaces may cause serious Newton's Ring pattern on final images. Examples of the data are shown for the cameras and the photometers based on the airglow observation at Shigaraki (35°N, 136°E), Japan.
url http://doi.org/10.15094/00009066
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