11:00 〜 11:15
[PEM12-26] ICON/MIGHTI as a Nightglow Probe of the Atomic Oxygen Green Line
キーワード：Airglow, Nightglow, Mesosphere, Photochemistry, Upper Atmosphere
The objective of the Michelson Interferometer for Global High-Resolution Thermospheric Imaging (MIGHTI) instrument aboard NASA’s Ionospheric Connection Explorer (ICON) satellite was to determine altitude profiles of the wind and temperature in the Earth’s upper atmosphere [1]. The winds were obtained from the Doppler shift of the measured atomic oxygen green and red line emissions at 557.7 nm and 630.0 nm [2], respectively, and the temperatures derived from the measured molecular oxygen Atmospheric band emission [3].
Our study aims to broaden the scientific impact of the MIGHTI instrument, advance knowledge of the nightglow emissions, and improve retrievals of nighttime atomic oxygen by using the intensities of the emissions measured by MIGHTI. Accurate nighttime O-atom densities are required for modeling the chemistry and energy budget of the upper atmosphere. Just as important, a detailed understanding of the relationship between atmospheric composition and the intensity of observed nightglow emissions is essential for modeling and understanding gravity wave propagation and dissipation.
We recently performed a radiometric calibration of the ICON/MIGHTI signals by comparisons with flux-calibrated astronomical sky spectra. This report will describe our efforts to investigate the calibrated 557.7-nm atomic oxygen green line emission measurements during the ICON/MIGHTI era, characterize its climatology, and determine atomic oxygen profiles.
This work is supported by the NASA GOLD-ICON Guest Investigators Program Grant 80NSSC22K0172 and the NASA Heliophysics (LNAPP) Program Grant 80NSSC23K0694.
[1] Immel et al., Space Sci. Rev. 219(41), 1-26 (2023).
[2] Englert et al., Space Sci. Rev. 219(3), 27 (2023).
[3] Stevens et al., Space Sci. Rev. 218(8), 67 (2022).
Our study aims to broaden the scientific impact of the MIGHTI instrument, advance knowledge of the nightglow emissions, and improve retrievals of nighttime atomic oxygen by using the intensities of the emissions measured by MIGHTI. Accurate nighttime O-atom densities are required for modeling the chemistry and energy budget of the upper atmosphere. Just as important, a detailed understanding of the relationship between atmospheric composition and the intensity of observed nightglow emissions is essential for modeling and understanding gravity wave propagation and dissipation.
We recently performed a radiometric calibration of the ICON/MIGHTI signals by comparisons with flux-calibrated astronomical sky spectra. This report will describe our efforts to investigate the calibrated 557.7-nm atomic oxygen green line emission measurements during the ICON/MIGHTI era, characterize its climatology, and determine atomic oxygen profiles.
This work is supported by the NASA GOLD-ICON Guest Investigators Program Grant 80NSSC22K0172 and the NASA Heliophysics (LNAPP) Program Grant 80NSSC23K0694.
[1] Immel et al., Space Sci. Rev. 219(41), 1-26 (2023).
[2] Englert et al., Space Sci. Rev. 219(3), 27 (2023).
[3] Stevens et al., Space Sci. Rev. 218(8), 67 (2022).