日本地球惑星科学連合2021年大会

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[E] ポスター発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM13] 太陽地球系結合過程の研究基盤形成

2021年6月4日(金) 17:15 〜 18:30 Ch.05

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

17:15 〜 18:30

[PEM13-P09] Optical calibration system of NIPR for aurora and airglow observations

*小川 泰信1,2,3、門倉 昭1,2,3、江尻 省1,2 (1.国立極地研究所、2.総合研究大学院大学、3.情報・システム研究機構 データサイエンス共同利用基盤施設)

キーワード:Aurora、Airglow、Calibration

Calibration of optical instruments is important for accurate measurement of the absolute emission intensity of aurora and airglow. The National Institute of Polar Research (NIPR), Japan, has been operating a facility for the optical calibration which consists of three independent calibration systems to share with collaborating researchers. This paper introduces an outline of the facility and specifications of each system, calibration procedures, and examples of calibration results. With this facility, we can obtain the calibration data for the absolute sensitivity of optical instruments with an accuracy of about 2% within a wavelength range between 420 and 1050 nm. In addition, it is possible to calibrate transmission of optical filters and also relative sensitivity of optical instruments as a function of wavelengths. Current facility, upgraded in 2012, has been used by many researchers to calibrate their various optical instruments.

Reference:
Ogawa, Y., A. Kadokura, M. K. Ejiri, Optical calibration system of NIPR for aurora and airglow observations, Polar Science, doi:10.1016/j.polar.2020.100570, 2020.