Rotational line intensities of the c4′1Σu+(1)-X1Σg+(0-2) bands of N2
Author:
Funder
National Research Division of the Spanish Ministry for Education
Publisher
Elsevier BV
Subject
Physical and Theoretical Chemistry,General Physics and Astronomy
Reference42 articles.
1. Extreme Ultraviolet Observations from Voyager 1 Encounter with Saturn
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3. Nitrogen airglow sources: Comparison of Triton, Titan, and Earth
4. Medium-resolution studies of extreme ultraviolet emission fromN2by electron impact: Vibrational perturbations and cross sections of thec4’Σu+1and b’Σu+1states
5. Absolute optical oscillator strengths for discrete and continuum photoabsorption of molecular nitrogen (11–200 eV)
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1. Opacities of <inline-formula><tex-math id="Z-20220715033133-1">\begin{document}${ X}^1\Sigma^+_{\rm g}, a'{}^1\Sigma^-_{\rm u}, a{}^1\Pi_{\rm g} \text{ and } { b}^1\Pi_{\rm u}$\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="14-20220043_Z-20220715033133-1.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="14-20220043_Z-20220715033133-1.png"/></alternatives></inline-formula> electronic states for nitrogen molecule;Acta Physica Sinica;2022
2. Theoretical Study of the Rotational Structure of the c4′1Σu + (6)–X1Σg +(0–9) Absorption Bands of N2;The Astrophysical Journal;2021-11-24
3. Line Oscillator Strengths for the c4′ 1Σu +(4)–X1Σg +(0–7) Absorption Bands of N2;The Astrophysical Journal;2020-08-12
4. Transition Energies and Absorption Oscillator Strengths for ${{c}_{4}}^{\prime 1}{{{\rm{\Sigma }}}_{u}}^{+}-{{\rm{X}}}^{1}{{{\rm{\Sigma }}}_{g}}^{+}$, ${b}^{\prime 1}{{{\rm{\Sigma }}}_{u}}^{+}-{{\rm{X}}}^{1}{{{\rm{\Sigma }}}_{g}}^{+}$, and ${{c}_{5}}^{\prime 1}{{{\rm{\Sigma }}}_{u}}^{+}-{{\rm{X}}}^{1}{{{\rm{\Sigma }}}_{g}}^{+}$ Band Systems in N 2;The Astrophysical Journal Supplement Series;2017-03-30
5. ABSORPTION OSCILLATOR STRENGTHS FOR THE c(4)(' 1)Sigma(+)(u)(3,4,6)-X-1 Sigma(+)(g)(nu ''), b(' 1)Sigma(+)(u)(10,13,20)-X-1 Sigma(+)(g)(nu ''), AND c(5)(' 1)Sigma(+)(u)(1)-X-1 Sigma(+)(g)(nu '') PROGRESSIONS IN N-2;ASTROPHYS J;2016
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