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High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry
A high-speed laser absorption technique is employed to resolve spectral transitions of CO[Formula: see text] in the mid-infrared at MHz rates to infer non-equilibrium populations/temperatures of translation, rotation and vibration in shock-heated CO[Formula: see text] - Ar mixtures. An interband cas...
Autores principales: | , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Berlin Heidelberg
2022
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9666324/ https://www.ncbi.nlm.nih.gov/pubmed/36407910 http://dx.doi.org/10.1007/s00340-022-07934-4 |
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author | Jelloian, Christopher C. Minesi, Nicolas Q. Spearrin, R. Mitchell |
author_facet | Jelloian, Christopher C. Minesi, Nicolas Q. Spearrin, R. Mitchell |
author_sort | Jelloian, Christopher C. |
collection | PubMed |
description | A high-speed laser absorption technique is employed to resolve spectral transitions of CO[Formula: see text] in the mid-infrared at MHz rates to infer non-equilibrium populations/temperatures of translation, rotation and vibration in shock-heated CO[Formula: see text] - Ar mixtures. An interband cascade laser (DFB-ICL) resolves 4 transitions within the CO[Formula: see text] asymmetric stretch fundamental bands ([Formula: see text] v[Formula: see text] = 1) near 4.19 [Formula: see text] . The sensor probes a wide range of rotational energies as well as two vibrational states (00[Formula: see text] 0 and 01[Formula: see text] 0). The sensor is demonstrated on the UCLA high enthalpy shock tube, targeting temperatures between 1250 and 3100 K and sub-atmospheric pressures (up to 0.2 atm). The sensor is sensitive to multiple temperatures over a wide range of conditions relevant to Mars entry radiation. Vibrational relaxation times are resolved and compared to existing models of thermal non-equilibrium. Select conditions highlight the shortcomings of modeling CO[Formula: see text] non-equilibrium with a single vibrational temperature. |
format | Online Article Text |
id | pubmed-9666324 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2022 |
publisher | Springer Berlin Heidelberg |
record_format | MEDLINE/PubMed |
spelling | pubmed-96663242022-11-17 High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry Jelloian, Christopher C. Minesi, Nicolas Q. Spearrin, R. Mitchell Appl Phys B Research A high-speed laser absorption technique is employed to resolve spectral transitions of CO[Formula: see text] in the mid-infrared at MHz rates to infer non-equilibrium populations/temperatures of translation, rotation and vibration in shock-heated CO[Formula: see text] - Ar mixtures. An interband cascade laser (DFB-ICL) resolves 4 transitions within the CO[Formula: see text] asymmetric stretch fundamental bands ([Formula: see text] v[Formula: see text] = 1) near 4.19 [Formula: see text] . The sensor probes a wide range of rotational energies as well as two vibrational states (00[Formula: see text] 0 and 01[Formula: see text] 0). The sensor is demonstrated on the UCLA high enthalpy shock tube, targeting temperatures between 1250 and 3100 K and sub-atmospheric pressures (up to 0.2 atm). The sensor is sensitive to multiple temperatures over a wide range of conditions relevant to Mars entry radiation. Vibrational relaxation times are resolved and compared to existing models of thermal non-equilibrium. Select conditions highlight the shortcomings of modeling CO[Formula: see text] non-equilibrium with a single vibrational temperature. Springer Berlin Heidelberg 2022-11-15 2022 /pmc/articles/PMC9666324/ /pubmed/36407910 http://dx.doi.org/10.1007/s00340-022-07934-4 Text en © The Author(s) 2022 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Research Jelloian, Christopher C. Minesi, Nicolas Q. Spearrin, R. Mitchell High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry |
title | High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry |
title_full | High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry |
title_fullStr | High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry |
title_full_unstemmed | High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry |
title_short | High-speed mid-infrared laser absorption spectroscopy of CO[Formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry |
title_sort | high-speed mid-infrared laser absorption spectroscopy of co[formula: see text] for shock-induced thermal non-equilibrium studies of planetary entry |
topic | Research |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9666324/ https://www.ncbi.nlm.nih.gov/pubmed/36407910 http://dx.doi.org/10.1007/s00340-022-07934-4 |
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