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- W3210702958 abstract "<p>We studied O<sub>2</sub> aurora based on the observations of O<sub>2</sub> emission at 1.27 &#956;m from the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument during the nighttime over 18 years. The horizontal structure and vertical profile of O<sub>2</sub> auroral volume emission rate is obtained after removing O<sub>2</sub> nightglow contamination. The O<sub>2</sub> auroral intensity varies between 0.14 and 5.97 kR, and the peak volume emission rate varies between 0.97 &#215; 10<sup>2</sup> and 41.01 &#215; 10<sup>2</sup> photons cm<sup>&#8722;3</sup> s<sup>&#8722;1</sup>. The O<sub>2 </sub>auroral intensity and peak volume emission rate exponentially increases with increasing Kp index, whereas the peak height decreases with increasing Kp index. The O<sub>2</sub> auroral intensity and peak volume emission rate under solar minimum condition are larger than those under solar maximum condition. The peak height under solar minimum condition is lower than that under solar maximum condition.</p>" @default.
- W3210702958 created "2021-11-08" @default.
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- W3210702958 date "2021-03-03" @default.
- W3210702958 modified "2023-09-26" @default.
- W3210702958 title "The O2 aurora observed by the TIMED/SABER satellite" @default.
- W3210702958 doi "https://doi.org/10.5194/egusphere-egu21-645" @default.
- W3210702958 hasPublicationYear "2021" @default.
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