EGU2020-4333
https://doi.org/10.5194/egusphere-egu2020-4333
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Estimating Boltzmann vibrational temperature of N2 (B^3Pi_g) using ISUAL 630nm, N2 1P (623-754 nm) and 762 nm-filtered imager data

Cheng Ling Kuo1,2 and the ISUAL Science Team*
Cheng Ling Kuo and the ISUAL Science Team
  • 1Institute of Space Science and Engineering, National Central University, Taoyuan, Taiwan (chengling.kuo@gmail.com)
  • 2Center for Astronautical Physics and Engineering, National Central University, Taoyuan, Taiwan
  • *A full list of authors appears at the end of the abstract

Multi-band observation of transient luminous events (TLEs) is one of the useful methodologies to be employed in sprite campaigns. Here, we show a method to estimate the Boltzmann vibrational temperature of N2 (B3Πg) by analyzing the 630nm-filtered, N2 1P-filtered and 762 nm-filtered images of TLEs. Our advanced method is validated in compassion with derived relative vibrational distributions by sprite spectrum (Kanmae et al., 2007). The imager recorded N2 1P-filtered emission (I1P,  623 – 754 nm) of TLEs indicates the intensity of N2 1P Δv=3 and partial with Δv=2 where dominated emissions with upper state vibrational number v=4, 5 and 6, i.e., N2 1P (4, 2), (4, 1), (5, 2) and (6, 3). The imager recorded 630 nm-filtered emissions (I630) were contributed primarily from N2 1P (10, 7) with v=10 while N2 1P (3, 1) for 762 nm-filtered emissions (I762) with v=3. Hence, we calculated the emission ratios of I630 to I1P, I630 to I762 and I762 to I1P. The emission ratios of I630 to I1P, I630 to I762 and I762 to I1P  also reflect the relative vibrational distributions of vibrational levels with LOW v=3 (I762), MIDDLE v=4, 5, 6 (I1P,  623 – 754 nm), and HIGH v=10 (I630). Therefore, we use the Boltzmann temperature for indicating the relative vibrational distributions of the specified group (LOW/MIDDLE/HIGH) of N2 (B3Πg) vibrational levels. For ISUAL recorded sprites, the average brightness of N2 1P (I1p), 762 nm (I762) and 630 nm (I630) emission was 2.3, 0.6 and 0.02 MR. The N2 (B3Πg) vibrational temperatures (Tv) were estimated to be 2800 K, 3200 K and 4300 K for multi-band emission ratios of I630/ I1p, I630/ I762 and I762/ I1p. For observed elves, the average brightness I1p, I762 and I630 were 170, 50 and 3 kR. The estimated Tv values were 3700 K, 3700 K and 3800 K for ratios I630/ I1p, I630/ I762 and I762/ I1p. For observed gigantic jets, the derived Tv values were 3000 – 5000 K for a ratio I762/ I1p. Through N2 (B3Πg) Tv analyses from emission ratios of ISUAL multi-band observation, we derived the N2 (B3Πg) vibrational temperature that ranges between 3000 and 5000 K or higher in TLEs. Accuracy and variations of derived N2 (B3Πg) Tv are also discussed while the relative population of vibrational levels in the Boltzmann equilibrium are also compared with past spectra observation. The details are shown in the publication (https://doi.org/10.1029/2019JA027311).

ISUAL Science Team:

Jung-Kuang Chou, Yen-Jung Wu, Earle Williams, Alfred B.-C. Chen, H. T. Su, R. R. Hsu, Harald U. Frey, Stephen B. Mende, and L. C. Lee

How to cite: Kuo, C. L. and the ISUAL Science Team: Estimating Boltzmann vibrational temperature of N2 (B^3Pi_g) using ISUAL 630nm, N2 1P (623-754 nm) and 762 nm-filtered imager data, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-4333, https://doi.org/10.5194/egusphere-egu2020-4333, 2020