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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1999-03-01
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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 |
work_keys_str_mv |
AT yasuokatoh calibrationofallskycamerasandtiltingphotometersusinganintegratingsphereandaspectrometer AT kazuoshiokawa calibrationofallskycamerasandtiltingphotometersusinganintegratingsphereandaspectrometer AT mitsugisatoh calibrationofallskycamerasandtiltingphotometersusinganintegratingsphereandaspectrometer AT mitsumukejiri calibrationofallskycamerasandtiltingphotometersusinganintegratingsphereandaspectrometer AT tadahikoogawa calibrationofallskycamerasandtiltingphotometersusinganintegratingsphereandaspectrometer |
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1725603847034896384 |