Theoretical Study of the Rotational Structure of the c4′1Σu + (6)–X1Σg +(0–9) Absorption Bands of N2

We have theoretically determined the absorption oscillator strengths and wavenumbers for rotationally resolved transitions of the c4′1Σu + (6)-X1Σg +(0–9) bands of N2, which are relevant to analyze the spectra of planetary atmospheres. The Molecular Quantum Defect Orbital method has been used in our...

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Veröffentlicht in:The Astrophysical journal 2021-12, Vol.922 (2)
Hauptverfasser: Velasco, A. M., Alonso, J. L., Redondo, P., Lavín, C.
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Sprache:eng
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