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

doi:10.1029/2012JA017599

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

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

13 引文斯高帕斯（Scopus）

摘要

[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 ³Π_g - A³Σ_u⁺), N₂ 2P(C³Π_u - B³Π_g), N₂ Lyman-Birge-Hopfield (a¹Π_g - X ¹Σ_g⁺), N₂⁺ 1N (B²Σ_u⁺ - X²S_g ⁺) and O₂⁺ 1N (b⁴Σ _g^- - a⁴Π_u) but also the post-impulse chemiluminescenses, O₂ atmospheric band (b ¹Σ_g⁺ - 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.

原文	???core.languages.en_GB???
文章編號	A07320
期刊	Journal of Geophysical Research: Space Physics
卷	117
發行號	7
DOIs	https://doi.org/10.1029/2012JA017599
出版狀態	已出版 - 2012

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10.1029/2012JA017599

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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. (2012). Full-kinetic elve model simulations and their comparisons with the ISUAL observed events. Journal of Geophysical Research: Space Physics, 117(7), 文章 A07320. https://doi.org/10.1029/2012JA017599

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title = "Full-kinetic elve model simulations and their comparisons with the ISUAL observed events",

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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doi = "10.1029/2012JA017599",

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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

Y1 - 2012

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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DO - 10.1029/2012JA017599

M3 - 期刊論文

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SN - 2169-9380

VL - 117

JO - Journal of Geophysical Research: Space Physics

JF - Journal of Geophysical Research: Space Physics

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M1 - A07320

ER -

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

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