The molecular oxygen 118-GHz line intensity revision

The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectr...
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Gespeichert in:

Autor*in:	Makarov, Dmitriy S. [verfasserIn] Serov, Evgeniy A. [verfasserIn] Galanina, Tatyana A. [verfasserIn] Koroleva, Aleksandra O. [verfasserIn] Tretyakov, Mikhail Yu. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption

Übergeordnetes Werk:	Enthalten in: Journal of molecular spectroscopy - Orlando, Fla. : Academic Press, 1957, 395
Übergeordnetes Werk:	volume:395

DOI / URN:	10.1016/j.jms.2023.111792

Katalog-ID:	ELV061414859

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245	1	0	\|a The molecular oxygen 118-GHz line intensity revision
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520			\|a The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large.
650		4	\|a Microwave spectroscopy
650		4	\|a Molecular oxygen
650		4	\|a Collisional coupling
650		4	\|a Line intensity
650		4	\|a Speed dependent effects
650		4	\|a Atmospheric absorption
700	1		\|a Serov, Evgeniy A. \|e verfasserin \|4 aut
700	1		\|a Galanina, Tatyana A. \|e verfasserin \|4 aut
700	1		\|a Koroleva, Aleksandra O. \|e verfasserin \|4 aut
700	1		\|a Tretyakov, Mikhail Yu. \|e verfasserin \|4 aut
773	0	8	\|i Enthalten in \|t Journal of molecular spectroscopy \|d Orlando, Fla. : Academic Press, 1957 \|g 395 \|h Online-Ressource \|w (DE-627)267328133 \|w (DE-600)1469771-3 \|w (DE-576)103815716 \|x 0022-2852 \|7 nnns
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allfields	10.1016/j.jms.2023.111792 doi (DE-627)ELV061414859 (ELSEVIER)S0022-2852(23)00057-7 DE-627 ger DE-627 rda eng 540 530 VZ 35.00 bkl Makarov, Dmitriy S. verfasserin aut The molecular oxygen 118-GHz line intensity revision 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large. Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption Serov, Evgeniy A. verfasserin aut Galanina, Tatyana A. verfasserin aut Koroleva, Aleksandra O. verfasserin aut Tretyakov, Mikhail Yu. verfasserin aut Enthalten in Journal of molecular spectroscopy Orlando, Fla. : Academic Press, 1957 395 Online-Ressource (DE-627)267328133 (DE-600)1469771-3 (DE-576)103815716 0022-2852 nnns volume:395 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 35.00 Chemie: Allgemeines VZ AR 395
spelling	10.1016/j.jms.2023.111792 doi (DE-627)ELV061414859 (ELSEVIER)S0022-2852(23)00057-7 DE-627 ger DE-627 rda eng 540 530 VZ 35.00 bkl Makarov, Dmitriy S. verfasserin aut The molecular oxygen 118-GHz line intensity revision 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large. Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption Serov, Evgeniy A. verfasserin aut Galanina, Tatyana A. verfasserin aut Koroleva, Aleksandra O. verfasserin aut Tretyakov, Mikhail Yu. verfasserin aut Enthalten in Journal of molecular spectroscopy Orlando, Fla. : Academic Press, 1957 395 Online-Ressource (DE-627)267328133 (DE-600)1469771-3 (DE-576)103815716 0022-2852 nnns volume:395 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 35.00 Chemie: Allgemeines VZ AR 395
allfields_unstemmed	10.1016/j.jms.2023.111792 doi (DE-627)ELV061414859 (ELSEVIER)S0022-2852(23)00057-7 DE-627 ger DE-627 rda eng 540 530 VZ 35.00 bkl Makarov, Dmitriy S. verfasserin aut The molecular oxygen 118-GHz line intensity revision 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large. Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption Serov, Evgeniy A. verfasserin aut Galanina, Tatyana A. verfasserin aut Koroleva, Aleksandra O. verfasserin aut Tretyakov, Mikhail Yu. verfasserin aut Enthalten in Journal of molecular spectroscopy Orlando, Fla. : Academic Press, 1957 395 Online-Ressource (DE-627)267328133 (DE-600)1469771-3 (DE-576)103815716 0022-2852 nnns volume:395 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 35.00 Chemie: Allgemeines VZ AR 395
allfieldsGer	10.1016/j.jms.2023.111792 doi (DE-627)ELV061414859 (ELSEVIER)S0022-2852(23)00057-7 DE-627 ger DE-627 rda eng 540 530 VZ 35.00 bkl Makarov, Dmitriy S. verfasserin aut The molecular oxygen 118-GHz line intensity revision 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large. Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption Serov, Evgeniy A. verfasserin aut Galanina, Tatyana A. verfasserin aut Koroleva, Aleksandra O. verfasserin aut Tretyakov, Mikhail Yu. verfasserin aut Enthalten in Journal of molecular spectroscopy Orlando, Fla. : Academic Press, 1957 395 Online-Ressource (DE-627)267328133 (DE-600)1469771-3 (DE-576)103815716 0022-2852 nnns volume:395 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 35.00 Chemie: Allgemeines VZ AR 395
allfieldsSound	10.1016/j.jms.2023.111792 doi (DE-627)ELV061414859 (ELSEVIER)S0022-2852(23)00057-7 DE-627 ger DE-627 rda eng 540 530 VZ 35.00 bkl Makarov, Dmitriy S. verfasserin aut The molecular oxygen 118-GHz line intensity revision 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large. Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption Serov, Evgeniy A. verfasserin aut Galanina, Tatyana A. verfasserin aut Koroleva, Aleksandra O. verfasserin aut Tretyakov, Mikhail Yu. verfasserin aut Enthalten in Journal of molecular spectroscopy Orlando, Fla. : Academic Press, 1957 395 Online-Ressource (DE-627)267328133 (DE-600)1469771-3 (DE-576)103815716 0022-2852 nnns volume:395 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 35.00 Chemie: Allgemeines VZ AR 395
language	English
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sourceStr	Enthalten in Journal of molecular spectroscopy 395 volume:395
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topic_facet	Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption
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container_title	Journal of molecular spectroscopy
authorswithroles_txt_mv	Makarov, Dmitriy S. @@aut@@ Serov, Evgeniy A. @@aut@@ Galanina, Tatyana A. @@aut@@ Koroleva, Aleksandra O. @@aut@@ Tretyakov, Mikhail Yu. @@aut@@
publishDateDaySort_date	2023-01-01T00:00:00Z
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author	Makarov, Dmitriy S.
spellingShingle	Makarov, Dmitriy S. ddc 540 bkl 35.00 misc Microwave spectroscopy misc Molecular oxygen misc Collisional coupling misc Line intensity misc Speed dependent effects misc Atmospheric absorption The molecular oxygen 118-GHz line intensity revision
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topic_title	540 530 VZ 35.00 bkl The molecular oxygen 118-GHz line intensity revision Microwave spectroscopy Molecular oxygen Collisional coupling Line intensity Speed dependent effects Atmospheric absorption
topic	ddc 540 bkl 35.00 misc Microwave spectroscopy misc Molecular oxygen misc Collisional coupling misc Line intensity misc Speed dependent effects misc Atmospheric absorption
topic_unstemmed	ddc 540 bkl 35.00 misc Microwave spectroscopy misc Molecular oxygen misc Collisional coupling misc Line intensity misc Speed dependent effects misc Atmospheric absorption
topic_browse	ddc 540 bkl 35.00 misc Microwave spectroscopy misc Molecular oxygen misc Collisional coupling misc Line intensity misc Speed dependent effects misc Atmospheric absorption
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title	The molecular oxygen 118-GHz line intensity revision
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title_full	The molecular oxygen 118-GHz line intensity revision
author_sort	Makarov, Dmitriy S.
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author_browse	Makarov, Dmitriy S. Serov, Evgeniy A. Galanina, Tatyana A. Koroleva, Aleksandra O. Tretyakov, Mikhail Yu.
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title_sort	the molecular oxygen 118-ghz line intensity revision
title_auth	The molecular oxygen 118-GHz line intensity revision
abstract	The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large.
abstractGer	The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large.
abstract_unstemmed	The intensity of the atmospheric diagnostic fine-structure line of the O 2 molecule at 118.75 GHz is revised based on multiple measurements with a resonator spectrometer in pure O 2 and O 2 –N 2 mixture at pressures ranging from 250 to 1500 Torr and temperatures within 278–327 K. The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. An excellent agreement with the result of calculations presented in HITRAN is demonstrated, suggesting that the 10%–20% uncertainty recommended by the database for all fine structure lines is too large.
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title_short	The molecular oxygen 118-GHz line intensity revision
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author2	Serov, Evgeniy A. Galanina, Tatyana A. Koroleva, Aleksandra O. Tretyakov, Mikhail Yu
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up_date	2024-07-06T17:37:46.487Z
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The resulting intensity of 1.000(3) ⋅ 1 0 − 25 cm/molec confirms the earlier measurements and allows decreasing the uncertainty down to ∼ 0.3%. 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The molecular oxygen 118-GHz line intensity revision

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