Full-kinetic elve model simulations and their comparisons with the ISUAL observed events

C. L. Kuo, T. Y. Huang, S. C. Chang, J. K. Chou, L. J. Lee, Y. J. Wu, A. B. Chen, H. T. Su, R. R. Hsu, H. U. Frey, S. B. Mende, Y. Takahashi, L. C. Lee

Research output: Contribution to journalArticle

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Abstract

[1] A full kinetic elve model with a wide time range from microseconds to seconds and its spectral range from UV, visible to near-infrared wavelengths is developed. Not only the fast electron-impact emissions N2 1P (B 3Πg - A3Σu+), N2 2P(C3Πu - B3Πg), N2 Lyman-Birge-Hopfield (a1Πg - X 1Σg+), N2+ 1N (B2Σu+ - X2Sg +) and O2+ 1N (b4Σ g- - a4Πu) but also the post-impulse chemiluminescenses, O2 atmospheric band (b 1Σg+ - X3Σ g-), O(1S - 1D) at 557.7 nm and O(1D - 3P) at 630 nm, are considered in the elve model. We calculate the dominant emissions and possible weak emissions in our elves model to analyze the relative importance of emission intensity, measured by the ISUAL imager with 5 selectable band pass filters (N21P, 762, 630, 557.7, 427.8 nm filter). The modeling emission intensities were well consistent with the measurements by Imager with different filters. This comparison could also be useful in designing the imager filters for future TLE survey missions in Earth orbit.

Original languageEnglish
Article numberA07320
JournalJournal of Geophysical Research: Space Physics
Volume117
Issue number7
DOIs
Publication statusPublished - 2012 Jan 1

Fingerprint

Image sensors
simulation models
kinetics
emissions factor
Kinetics
filter
simulation
filters
Bandpass filters
elves
orbits
Orbits
Earth (planet)
Earth orbits
Infrared radiation
wavelengths
Wavelength
bandpass filters
Electrons
electrons

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

Cite this

Kuo, C. L., Huang, T. Y., Chang, S. C., Chou, J. K., Lee, L. J., Wu, Y. J., ... Lee, L. C. (2012). Full-kinetic elve model simulations and their comparisons with the ISUAL observed events. Journal of Geophysical Research: Space Physics, 117(7), [A07320]. https://doi.org/10.1029/2012JA017599
Kuo, C. L. ; Huang, T. Y. ; Chang, S. C. ; Chou, J. K. ; Lee, L. J. ; Wu, Y. J. ; Chen, A. B. ; Su, H. T. ; Hsu, R. R. ; Frey, H. U. ; Mende, S. B. ; Takahashi, Y. ; Lee, L. C. / Full-kinetic elve model simulations and their comparisons with the ISUAL observed events. In: Journal of Geophysical Research: Space Physics. 2012 ; Vol. 117, No. 7.
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abstract = "[1] A full kinetic elve model with a wide time range from microseconds to seconds and its spectral range from UV, visible to near-infrared wavelengths is developed. Not only the fast electron-impact emissions N2 1P (B 3Πg - A3Σu+), N2 2P(C3Πu - B3Πg), N2 Lyman-Birge-Hopfield (a1Πg - X 1Σg+), N2+ 1N (B2Σu+ - X2Sg +) and O2+ 1N (b4Σ g- - a4Πu) but also the post-impulse chemiluminescenses, O2 atmospheric band (b 1Σg+ - X3Σ g-), O(1S - 1D) at 557.7 nm and O(1D - 3P) at 630 nm, are considered in the elve model. We calculate the dominant emissions and possible weak emissions in our elves model to analyze the relative importance of emission intensity, measured by the ISUAL imager with 5 selectable band pass filters (N21P, 762, 630, 557.7, 427.8 nm filter). The modeling emission intensities were well consistent with the measurements by Imager with different filters. This comparison could also be useful in designing the imager filters for future TLE survey missions in Earth orbit.",
author = "Kuo, {C. L.} and Huang, {T. Y.} and Chang, {S. C.} and Chou, {J. K.} and Lee, {L. J.} and Wu, {Y. J.} and Chen, {A. B.} and Su, {H. T.} and Hsu, {R. R.} and Frey, {H. U.} and Mende, {S. B.} and Y. Takahashi and Lee, {L. C.}",
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Kuo, CL, Huang, TY, Chang, SC, Chou, JK, Lee, LJ, Wu, YJ, Chen, AB, Su, HT, Hsu, RR, Frey, HU, Mende, SB, Takahashi, Y & Lee, LC 2012, 'Full-kinetic elve model simulations and their comparisons with the ISUAL observed events', Journal of Geophysical Research: Space Physics, vol. 117, no. 7, A07320. https://doi.org/10.1029/2012JA017599

Full-kinetic elve model simulations and their comparisons with the ISUAL observed events. / Kuo, C. L.; Huang, T. Y.; Chang, S. C.; Chou, J. K.; Lee, L. J.; Wu, Y. J.; Chen, A. B.; Su, H. T.; Hsu, R. R.; Frey, H. U.; Mende, S. B.; Takahashi, Y.; Lee, L. C.

In: Journal of Geophysical Research: Space Physics, Vol. 117, No. 7, A07320, 01.01.2012.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Full-kinetic elve model simulations and their comparisons with the ISUAL observed events

AU - Kuo, C. L.

AU - Huang, T. Y.

AU - Chang, S. C.

AU - Chou, J. K.

AU - Lee, L. J.

AU - Wu, Y. J.

AU - Chen, A. B.

AU - Su, H. T.

AU - Hsu, R. R.

AU - Frey, H. U.

AU - Mende, S. B.

AU - Takahashi, Y.

AU - Lee, L. C.

PY - 2012/1/1

Y1 - 2012/1/1

N2 - [1] A full kinetic elve model with a wide time range from microseconds to seconds and its spectral range from UV, visible to near-infrared wavelengths is developed. Not only the fast electron-impact emissions N2 1P (B 3Πg - A3Σu+), N2 2P(C3Πu - B3Πg), N2 Lyman-Birge-Hopfield (a1Πg - X 1Σg+), N2+ 1N (B2Σu+ - X2Sg +) and O2+ 1N (b4Σ g- - a4Πu) but also the post-impulse chemiluminescenses, O2 atmospheric band (b 1Σg+ - X3Σ g-), O(1S - 1D) at 557.7 nm and O(1D - 3P) at 630 nm, are considered in the elve model. We calculate the dominant emissions and possible weak emissions in our elves model to analyze the relative importance of emission intensity, measured by the ISUAL imager with 5 selectable band pass filters (N21P, 762, 630, 557.7, 427.8 nm filter). The modeling emission intensities were well consistent with the measurements by Imager with different filters. This comparison could also be useful in designing the imager filters for future TLE survey missions in Earth orbit.

AB - [1] A full kinetic elve model with a wide time range from microseconds to seconds and its spectral range from UV, visible to near-infrared wavelengths is developed. Not only the fast electron-impact emissions N2 1P (B 3Πg - A3Σu+), N2 2P(C3Πu - B3Πg), N2 Lyman-Birge-Hopfield (a1Πg - X 1Σg+), N2+ 1N (B2Σu+ - X2Sg +) and O2+ 1N (b4Σ g- - a4Πu) but also the post-impulse chemiluminescenses, O2 atmospheric band (b 1Σg+ - X3Σ g-), O(1S - 1D) at 557.7 nm and O(1D - 3P) at 630 nm, are considered in the elve model. We calculate the dominant emissions and possible weak emissions in our elves model to analyze the relative importance of emission intensity, measured by the ISUAL imager with 5 selectable band pass filters (N21P, 762, 630, 557.7, 427.8 nm filter). The modeling emission intensities were well consistent with the measurements by Imager with different filters. This comparison could also be useful in designing the imager filters for future TLE survey missions in Earth orbit.

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