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The ammonia absorption spectrum revisited between 5650 and 6350 cm-1
- 1.0578228 - ÚFCH JH 2025 RIV GB eng J - Journal Article
Cacciani, P. - Čermák, P. - Votava, Ondřej - Vander Auwera, J. - Campargue, A.
The ammonia absorption spectrum revisited between 5650 and 6350 cm-1.
Molecular Physics. Roč. 122, 7-8 (2024), č. článku e2256893. ISSN 0026-8976. E-ISSN 1362-3028
Institutional support: RVO:61388955
Keywords : Ammonia * absorption spectroscopy * near infrared
OECD category: Physical chemistry
Impact factor: 1.6, year: 2023 ; AIS: 0.349, rok: 2023
Method of publishing: Limited access
Result website:
https://www.tandfonline.com/doi/abs/10.1080/00268976.2023.2256893DOI: https://doi.org/10.1080/00268976.2023.2256893
The ammonia spectrum is revisited in the important 1.6 mu m atmospheric transparency window between 5650 and 6350 cm(-1) on the basis of recently recorded high-resolution Fourier transform spectra. These spectra offer an improved frequency sampling and better traceability of the measurement conditions compared to previously studied Kitt Peak spectra (Cacciani et al. J. Quant Spectrosc Radiat Transf 2021, 258:107334. https://doi.org/10.1016/j.jqsrt.2020.107334). Overall, 4812 (NH3)-N-14 lines were measured in the 5650-6350 cm(-1) region corresponding to 4866 transitions including 2066 new ones compared with our previous study, included in the HITRAN2020 database. The energy of 1023 upper state levels (including 107 new ones) was derived from 2608 assigned transitions. Independently, ammonia spectra recorded in a supersonic jet expansion using a tunable extended cavity diode laser allow us to check the absolute transition energies in the 5980-6080 cm(-1) range. Accurate jet spectra calibration was achieved using CH4 reference line positions known with kHz accuracy. The position agreement with the FTS data is within the 4 x 10(-4) cm(-1) uncertainty of the positions measured in the jet expansion. A recommended line list of 5620 transitions is provided for (NH3)-N-14 in the considered 5650- 6350 cm(-1) region.
Permanent Link: https://hdl.handle.net/11104/0347252File Download Size Commentary Version Access 0578228preprint.pdf 0 26.5 MB Author´s preprint open-access
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