Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station

<p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p< Ausführliche Beschreibung

Gespeichert in:

Autor*in:	T. Fujinawa [verfasserIn] T. O. Sato [verfasserIn] T. Yamada [verfasserIn] S. Nara [verfasserIn] Y. Uchiyama [verfasserIn] K. Takahashi [verfasserIn] N. Yoshida [verfasserIn] Y. Kasai [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2020

Übergeordnetes Werk:	In: Atmospheric Measurement Techniques - Copernicus Publications, 2009, 13(2020), Seite 2119-2129
Übergeordnetes Werk:	volume:13 ; year:2020 ; pages:2119-2129

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc Journal toc

DOI / URN:	10.5194/amt-13-2119-2020

Katalog-ID:	DOAJ033021295

Internformat


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245	1	0	\|a Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station
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520			\|a <p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p<
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653		0	\|a Earthwork. Foundations
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700	0		\|a T. O. Sato \|e verfasserin \|4 aut
700	0		\|a T. Yamada \|e verfasserin \|4 aut
700	0		\|a S. Nara \|e verfasserin \|4 aut
700	0		\|a S. Nara \|e verfasserin \|4 aut
700	0		\|a Y. Uchiyama \|e verfasserin \|4 aut
700	0		\|a Y. Uchiyama \|e verfasserin \|4 aut
700	0		\|a K. Takahashi \|e verfasserin \|4 aut
700	0		\|a K. Takahashi \|e verfasserin \|4 aut
700	0		\|a N. Yoshida \|e verfasserin \|4 aut
700	0		\|a Y. Kasai \|e verfasserin \|4 aut
700	0		\|a Y. Kasai \|e verfasserin \|4 aut
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912			\|a GBV_ILN_4324
912			\|a GBV_ILN_4325
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951			\|a AR
952			\|d 13 \|j 2020 \|h 2119-2129

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author_variant	t f tf t f tf t o s tos t y ty s n sn s n sn y u yu y u yu k t kt k t kt n y ny y k yk y k yk
matchkey_str	article:18678548:2020----::aiainfctntiehu3ucmaueetitetaopeenlwreopeermhsieis
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allfields	10.5194/amt-13-2119-2020 doi (DE-627)DOAJ033021295 (DE-599)DOAJfb22c368b25b4e5d8fa24221f305dafa DE-627 ger DE-627 rakwb eng TA170-171 TA715-787 T. Fujinawa verfasserin aut Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier <p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p< Environmental engineering Earthwork. Foundations T. Fujinawa verfasserin aut T. O. Sato verfasserin aut T. Yamada verfasserin aut S. Nara verfasserin aut S. Nara verfasserin aut Y. Uchiyama verfasserin aut Y. Uchiyama verfasserin aut K. Takahashi verfasserin aut K. Takahashi verfasserin aut N. Yoshida verfasserin aut Y. Kasai verfasserin aut Y. Kasai verfasserin aut In Atmospheric Measurement Techniques Copernicus Publications, 2009 13(2020), Seite 2119-2129 (DE-627)605214441 (DE-600)2505596-3 18678548 nnns volume:13 year:2020 pages:2119-2129 https://doi.org/10.5194/amt-13-2119-2020 kostenfrei https://doaj.org/article/fb22c368b25b4e5d8fa24221f305dafa kostenfrei https://www.atmos-meas-tech.net/13/2119/2020/amt-13-2119-2020.pdf kostenfrei https://doaj.org/toc/1867-1381 Journal toc kostenfrei https://doaj.org/toc/1867-8548 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2020 2119-2129
spelling	10.5194/amt-13-2119-2020 doi (DE-627)DOAJ033021295 (DE-599)DOAJfb22c368b25b4e5d8fa24221f305dafa DE-627 ger DE-627 rakwb eng TA170-171 TA715-787 T. Fujinawa verfasserin aut Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier <p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p< Environmental engineering Earthwork. Foundations T. Fujinawa verfasserin aut T. O. Sato verfasserin aut T. Yamada verfasserin aut S. Nara verfasserin aut S. Nara verfasserin aut Y. Uchiyama verfasserin aut Y. Uchiyama verfasserin aut K. Takahashi verfasserin aut K. Takahashi verfasserin aut N. Yoshida verfasserin aut Y. Kasai verfasserin aut Y. Kasai verfasserin aut In Atmospheric Measurement Techniques Copernicus Publications, 2009 13(2020), Seite 2119-2129 (DE-627)605214441 (DE-600)2505596-3 18678548 nnns volume:13 year:2020 pages:2119-2129 https://doi.org/10.5194/amt-13-2119-2020 kostenfrei https://doaj.org/article/fb22c368b25b4e5d8fa24221f305dafa kostenfrei https://www.atmos-meas-tech.net/13/2119/2020/amt-13-2119-2020.pdf kostenfrei https://doaj.org/toc/1867-1381 Journal toc kostenfrei https://doaj.org/toc/1867-8548 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2020 2119-2129
allfields_unstemmed	10.5194/amt-13-2119-2020 doi (DE-627)DOAJ033021295 (DE-599)DOAJfb22c368b25b4e5d8fa24221f305dafa DE-627 ger DE-627 rakwb eng TA170-171 TA715-787 T. Fujinawa verfasserin aut Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier <p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p< Environmental engineering Earthwork. Foundations T. Fujinawa verfasserin aut T. O. Sato verfasserin aut T. Yamada verfasserin aut S. Nara verfasserin aut S. Nara verfasserin aut Y. Uchiyama verfasserin aut Y. Uchiyama verfasserin aut K. Takahashi verfasserin aut K. Takahashi verfasserin aut N. Yoshida verfasserin aut Y. Kasai verfasserin aut Y. Kasai verfasserin aut In Atmospheric Measurement Techniques Copernicus Publications, 2009 13(2020), Seite 2119-2129 (DE-627)605214441 (DE-600)2505596-3 18678548 nnns volume:13 year:2020 pages:2119-2129 https://doi.org/10.5194/amt-13-2119-2020 kostenfrei https://doaj.org/article/fb22c368b25b4e5d8fa24221f305dafa kostenfrei https://www.atmos-meas-tech.net/13/2119/2020/amt-13-2119-2020.pdf kostenfrei https://doaj.org/toc/1867-1381 Journal toc kostenfrei https://doaj.org/toc/1867-8548 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2020 2119-2129
allfieldsGer	10.5194/amt-13-2119-2020 doi (DE-627)DOAJ033021295 (DE-599)DOAJfb22c368b25b4e5d8fa24221f305dafa DE-627 ger DE-627 rakwb eng TA170-171 TA715-787 T. Fujinawa verfasserin aut Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier <p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p< Environmental engineering Earthwork. Foundations T. Fujinawa verfasserin aut T. O. Sato verfasserin aut T. Yamada verfasserin aut S. Nara verfasserin aut S. Nara verfasserin aut Y. Uchiyama verfasserin aut Y. Uchiyama verfasserin aut K. Takahashi verfasserin aut K. Takahashi verfasserin aut N. Yoshida verfasserin aut Y. Kasai verfasserin aut Y. Kasai verfasserin aut In Atmospheric Measurement Techniques Copernicus Publications, 2009 13(2020), Seite 2119-2129 (DE-627)605214441 (DE-600)2505596-3 18678548 nnns volume:13 year:2020 pages:2119-2129 https://doi.org/10.5194/amt-13-2119-2020 kostenfrei https://doaj.org/article/fb22c368b25b4e5d8fa24221f305dafa kostenfrei https://www.atmos-meas-tech.net/13/2119/2020/amt-13-2119-2020.pdf kostenfrei https://doaj.org/toc/1867-1381 Journal toc kostenfrei https://doaj.org/toc/1867-8548 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2020 2119-2129
allfieldsSound	10.5194/amt-13-2119-2020 doi (DE-627)DOAJ033021295 (DE-599)DOAJfb22c368b25b4e5d8fa24221f305dafa DE-627 ger DE-627 rakwb eng TA170-171 TA715-787 T. Fujinawa verfasserin aut Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier <p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p< Environmental engineering Earthwork. Foundations T. Fujinawa verfasserin aut T. O. Sato verfasserin aut T. Yamada verfasserin aut S. Nara verfasserin aut S. Nara verfasserin aut Y. Uchiyama verfasserin aut Y. Uchiyama verfasserin aut K. Takahashi verfasserin aut K. Takahashi verfasserin aut N. Yoshida verfasserin aut Y. Kasai verfasserin aut Y. Kasai verfasserin aut In Atmospheric Measurement Techniques Copernicus Publications, 2009 13(2020), Seite 2119-2129 (DE-627)605214441 (DE-600)2505596-3 18678548 nnns volume:13 year:2020 pages:2119-2129 https://doi.org/10.5194/amt-13-2119-2020 kostenfrei https://doaj.org/article/fb22c368b25b4e5d8fa24221f305dafa kostenfrei https://www.atmos-meas-tech.net/13/2119/2020/amt-13-2119-2020.pdf kostenfrei https://doaj.org/toc/1867-1381 Journal toc kostenfrei https://doaj.org/toc/1867-8548 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2020 2119-2129
language	English
source	In Atmospheric Measurement Techniques 13(2020), Seite 2119-2129 volume:13 year:2020 pages:2119-2129
sourceStr	In Atmospheric Measurement Techniques 13(2020), Seite 2119-2129 volume:13 year:2020 pages:2119-2129
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Environmental engineering Earthwork. Foundations
isfreeaccess_bool	true
container_title	Atmospheric Measurement Techniques
authorswithroles_txt_mv	T. Fujinawa @@aut@@ T. O. Sato @@aut@@ T. Yamada @@aut@@ S. Nara @@aut@@ Y. Uchiyama @@aut@@ K. Takahashi @@aut@@ N. Yoshida @@aut@@ Y. Kasai @@aut@@
publishDateDaySort_date	2020-01-01T00:00:00Z
hierarchy_top_id	605214441
id	DOAJ033021295
language_de	englisch
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Fujinawa</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a"><p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p<</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Environmental engineering</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Earthwork. Foundations</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. Fujinawa</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. O. Sato</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. Yamada</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Nara</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Nara</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Y. Uchiyama</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Y. Uchiyama</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">K. 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callnumber-first	T - Technology
author	T. Fujinawa
spellingShingle	T. Fujinawa misc TA170-171 misc TA715-787 misc Environmental engineering misc Earthwork. Foundations Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station
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topic_title	TA170-171 TA715-787 Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station
topic	misc TA170-171 misc TA715-787 misc Environmental engineering misc Earthwork. Foundations
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title	Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station
ctrlnum	(DE-627)DOAJ033021295 (DE-599)DOAJfb22c368b25b4e5d8fa24221f305dafa
title_full	Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station
author_sort	T. Fujinawa
journal	Atmospheric Measurement Techniques
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author_browse	T. Fujinawa T. O. Sato T. Yamada S. Nara Y. Uchiyama K. Takahashi N. Yoshida Y. Kasai
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author-letter	T. Fujinawa
doi_str_mv	10.5194/amt-13-2119-2020
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title_sort	validation of acetonitrile (ch<sub<3</sub<cn) measurements in the stratosphere and lower mesosphere from the smiles instrument on the international space station
callnumber	TA170-171
title_auth	Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station
abstract	<p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p<
abstractGer	<p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p<
abstract_unstemmed	<p<Acetonitrile (<span class="inline-formula"<CH<sub<3</sub<CN</span<) is a volatile organic compound (VOC) and a potential tracer of biomass burning. We evaluated the capability of using observations derived from the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the International Space Station (ISS) to measure <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles. The error in a <span class="inline-formula"<CH<sub<3</sub<CN</span< vertical profile from the Level-2 research (L2r) product version 3.0.0 was estimated by theoretical error analysis and also compared with other instrumental measurements. We estimated the systematic and random errors to be <span class="inline-formula"<∼5.8</span< ppt (7.8 %) and 25 ppt (60 %), respectively, for a single observation at 15.7 hPa in the tropics, where the <span class="inline-formula"<CH<sub<3</sub<CN</span< measurements are enhanced. The major source of systematic error was the pressure-broadening coefficient, and its contribution to the total systematic error was approximately 60 % in the middle stratosphere (15.7–4.8 hPa). The random error decreased to less than 40 % after averaging 10 profiles in the pressure range of 28.8–1.6 hPa. The total error due to uncertainties in other molecular spectroscopic parameters (2.8 ppt) was comparable to that of <span class="inline-formula"<CH<sub<3</sub<CN</span< spectroscopic parameters. We compared the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles with those of the microwave limb sounder (MLS) on the Aura satellite (version 4.2). The SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< values were consistent with those from MLS within the standard deviation (<span class="inline-formula"<1<i<σ</i<</span<) of the MLS observations. The difference between the SMILES and MLS <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles increased with altitude and was within 20–35 ppt (20 %–260 %) at 15.7–1.6 hPa. We observed discrepancies of 5–10 ppt (10 %–30 %) between the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles observed by different spectrometers, and hence, we do not recommend merging SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< profiles derived from different spectrometers. We found that the SMILES <span class="inline-formula"<CH<sub<3</sub<CN</span< volume mixing ratio (VMR) in the upper stratosphere has a seasonal maximum in February.</p<
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title_short	Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station
url	https://doi.org/10.5194/amt-13-2119-2020 https://doaj.org/article/fb22c368b25b4e5d8fa24221f305dafa https://www.atmos-meas-tech.net/13/2119/2020/amt-13-2119-2020.pdf https://doaj.org/toc/1867-1381 https://doaj.org/toc/1867-8548
remote_bool	true
author2	T. Fujinawa T. O. Sato T. Yamada S. Nara Y. Uchiyama K. Takahashi N. Yoshida Y. Kasai
author2Str	T. Fujinawa T. O. Sato T. Yamada S. Nara Y. Uchiyama K. Takahashi N. Yoshida Y. Kasai
ppnlink	605214441
callnumber-subject	TA - General and Civil Engineering
mediatype_str_mv	c
isOA_txt	true
hochschulschrift_bool	false
doi_str	10.5194/amt-13-2119-2020
callnumber-a	TA170-171
up_date	2024-07-03T15:23:44.995Z
_version_	1803571927445405696
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Validation of acetonitrile (CH<sub<3</sub<CN) measurements in the stratosphere and lower mesosphere from the SMILES instrument on the International Space Station

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