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Stratospheric ozone isotope enrichment studied by submillimeter wave heterodyne radiometry: the observation capabilities of SMILES
The isotopic ratio of molecules often provides valuable information about past or presently occurring processes in the atmosphere because chemical and physical processes may give rise to isotope fractionation of molecular species. However, there are so far no published satellite measurements on the...
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Published in: | IEEE transactions on geoscience and remote sensing 2006-03, Vol.44 (3), p.676-693 |
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description | The isotopic ratio of molecules often provides valuable information about past or presently occurring processes in the atmosphere because chemical and physical processes may give rise to isotope fractionation of molecular species. However, there are so far no published satellite measurements on the spatial and temporal variations of ozone isotopes in the stratosphere. Spectroscopic remote sensing methods can theoretically be used to observe ozone isotope fractionation on a global scale, but sufficient accuracy has not yet been achieved. A new generation of submillimeter-wave receivers employing sensitive superconductor-insulator-superconductor (SIS) detector technology will provide new opportunities for precise remote sensing measurements of ozone isotopes on a global scale. We have estimated the observation capabilities of two different SIS instruments, namely the space-station-borne Japanese Experimental Module/Sub-Millimeter-wave Limb Emission Sounder (JEM/SMILES) instrument, currently planned for launch in 2008, as well as the airborne Submillimeter wave Atmospheric Sounder/Airborne Submillimeter SIS Radiometer (SUMAS/ASUR) sensor. Measurements of the airborne sensor, conducted in 1996, are presented in order to demonstrate the detection of normal-O/sub 3/ and asymmetric-18-O/sub 3/ in the SMILES frequency bands. In the ideal case, JEM/SMILES has the capability to measure the ozone isotope enrichment (/spl delta//sup M/O/sub 3/) in the middle stratosphere with a precision of /spl sim/12/sup 0///sub 00/, /spl sim/11/sup 0///sub 00/, and /spl sim/9/sup 0///sub 00/, for asymmetric-18-O/sub 3/, symmetric-17-O/sub 3/, asymmetric-17-O/sub 3/, respectively, for a daily zonal mean product with resolution of 10/spl deg/ in latitude. The systematic error, including contributions of all instrumental and spectroscopic uncertainties, is estimated to be of the order of 100/sup 0///sub 00/ to 200/sup 0///sub 00/ and should be reduced by prelaunch laboratory measurements and in-flight calibrations. A remaining bias in the SMILES measurements will have to be quantified by dedicated validation campaigns. JEM/SMILES should then be capable to provide valuable information on the global distribution and seasonal variation of ozone isotope fractionation in the stratosphere. This new technology will allow us to shed new light on this still open issue in atmospheric sciences. |
doi_str_mv | 10.1109/TGRS.2005.861754 |
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However, there are so far no published satellite measurements on the spatial and temporal variations of ozone isotopes in the stratosphere. Spectroscopic remote sensing methods can theoretically be used to observe ozone isotope fractionation on a global scale, but sufficient accuracy has not yet been achieved. A new generation of submillimeter-wave receivers employing sensitive superconductor-insulator-superconductor (SIS) detector technology will provide new opportunities for precise remote sensing measurements of ozone isotopes on a global scale. We have estimated the observation capabilities of two different SIS instruments, namely the space-station-borne Japanese Experimental Module/Sub-Millimeter-wave Limb Emission Sounder (JEM/SMILES) instrument, currently planned for launch in 2008, as well as the airborne Submillimeter wave Atmospheric Sounder/Airborne Submillimeter SIS Radiometer (SUMAS/ASUR) sensor. Measurements of the airborne sensor, conducted in 1996, are presented in order to demonstrate the detection of normal-O/sub 3/ and asymmetric-18-O/sub 3/ in the SMILES frequency bands. In the ideal case, JEM/SMILES has the capability to measure the ozone isotope enrichment (/spl delta//sup M/O/sub 3/) in the middle stratosphere with a precision of /spl sim/12/sup 0///sub 00/, /spl sim/11/sup 0///sub 00/, and /spl sim/9/sup 0///sub 00/, for asymmetric-18-O/sub 3/, symmetric-17-O/sub 3/, asymmetric-17-O/sub 3/, respectively, for a daily zonal mean product with resolution of 10/spl deg/ in latitude. The systematic error, including contributions of all instrumental and spectroscopic uncertainties, is estimated to be of the order of 100/sup 0///sub 00/ to 200/sup 0///sub 00/ and should be reduced by prelaunch laboratory measurements and in-flight calibrations. A remaining bias in the SMILES measurements will have to be quantified by dedicated validation campaigns. JEM/SMILES should then be capable to provide valuable information on the global distribution and seasonal variation of ozone isotope fractionation in the stratosphere. This new technology will allow us to shed new light on this still open issue in atmospheric sciences.</description><identifier>ISSN: 0196-2892</identifier><identifier>EISSN: 1558-0644</identifier><identifier>DOI: 10.1109/TGRS.2005.861754</identifier><identifier>CODEN: IGRSD2</identifier><language>eng</language><publisher>New York, NY: IEEE</publisher><subject>Acoustic sensors ; Airborne sensing ; Applied geophysics ; Asymmetry ; Atmospheric measurements ; Atmospheric profiles retrieval ; Atmospheric sciences ; Atmospherics ; Carbon ; Chemical processes ; Earth sciences ; Earth, ocean, space ; Exact sciences and technology ; Fractionation ; Instruments ; Internal geophysics ; Isotopes ; limb sounder ; microwave spectroscopy ; Ozone ; Radiometry ; Remote sensing ; Spectroscopy ; Stratosphere ; stratospheric chemistry ; submillimeter wavelength ; superconducting receiver ; Terrestrial atmosphere</subject><ispartof>IEEE transactions on geoscience and remote sensing, 2006-03, Vol.44 (3), p.676-693</ispartof><rights>2006 INIST-CNRS</rights><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. (IEEE) 2006</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c428t-4451894b145bd02f366b832766fd45f40c1094d82372a435d8e8b235600732ef3</citedby><cites>FETCH-LOGICAL-c428t-4451894b145bd02f366b832766fd45f40c1094d82372a435d8e8b235600732ef3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/1597473$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,54796</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=17559078$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Kasai, Y.J.</creatorcontrib><creatorcontrib>Urban, J.</creatorcontrib><creatorcontrib>Takahashi, C.</creatorcontrib><creatorcontrib>Hoshino, S.</creatorcontrib><creatorcontrib>Takahashi, K.</creatorcontrib><creatorcontrib>Inatani, J.</creatorcontrib><creatorcontrib>Shiotani, M.</creatorcontrib><creatorcontrib>Masuko, H.</creatorcontrib><title>Stratospheric ozone isotope enrichment studied by submillimeter wave heterodyne radiometry: the observation capabilities of SMILES</title><title>IEEE transactions on geoscience and remote sensing</title><addtitle>TGRS</addtitle><description>The isotopic ratio of molecules often provides valuable information about past or presently occurring processes in the atmosphere because chemical and physical processes may give rise to isotope fractionation of molecular species. However, there are so far no published satellite measurements on the spatial and temporal variations of ozone isotopes in the stratosphere. Spectroscopic remote sensing methods can theoretically be used to observe ozone isotope fractionation on a global scale, but sufficient accuracy has not yet been achieved. A new generation of submillimeter-wave receivers employing sensitive superconductor-insulator-superconductor (SIS) detector technology will provide new opportunities for precise remote sensing measurements of ozone isotopes on a global scale. We have estimated the observation capabilities of two different SIS instruments, namely the space-station-borne Japanese Experimental Module/Sub-Millimeter-wave Limb Emission Sounder (JEM/SMILES) instrument, currently planned for launch in 2008, as well as the airborne Submillimeter wave Atmospheric Sounder/Airborne Submillimeter SIS Radiometer (SUMAS/ASUR) sensor. Measurements of the airborne sensor, conducted in 1996, are presented in order to demonstrate the detection of normal-O/sub 3/ and asymmetric-18-O/sub 3/ in the SMILES frequency bands. In the ideal case, JEM/SMILES has the capability to measure the ozone isotope enrichment (/spl delta//sup M/O/sub 3/) in the middle stratosphere with a precision of /spl sim/12/sup 0///sub 00/, /spl sim/11/sup 0///sub 00/, and /spl sim/9/sup 0///sub 00/, for asymmetric-18-O/sub 3/, symmetric-17-O/sub 3/, asymmetric-17-O/sub 3/, respectively, for a daily zonal mean product with resolution of 10/spl deg/ in latitude. The systematic error, including contributions of all instrumental and spectroscopic uncertainties, is estimated to be of the order of 100/sup 0///sub 00/ to 200/sup 0///sub 00/ and should be reduced by prelaunch laboratory measurements and in-flight calibrations. A remaining bias in the SMILES measurements will have to be quantified by dedicated validation campaigns. JEM/SMILES should then be capable to provide valuable information on the global distribution and seasonal variation of ozone isotope fractionation in the stratosphere. This new technology will allow us to shed new light on this still open issue in atmospheric sciences.</description><subject>Acoustic sensors</subject><subject>Airborne sensing</subject><subject>Applied geophysics</subject><subject>Asymmetry</subject><subject>Atmospheric measurements</subject><subject>Atmospheric profiles retrieval</subject><subject>Atmospheric sciences</subject><subject>Atmospherics</subject><subject>Carbon</subject><subject>Chemical processes</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Fractionation</subject><subject>Instruments</subject><subject>Internal geophysics</subject><subject>Isotopes</subject><subject>limb sounder</subject><subject>microwave spectroscopy</subject><subject>Ozone</subject><subject>Radiometry</subject><subject>Remote sensing</subject><subject>Spectroscopy</subject><subject>Stratosphere</subject><subject>stratospheric chemistry</subject><subject>submillimeter wavelength</subject><subject>superconducting receiver</subject><subject>Terrestrial atmosphere</subject><issn>0196-2892</issn><issn>1558-0644</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqFks9r1EAUx4MouFbvgpdB0HrJ-ub3pDcptRZWBLeewyR5YackmXVmUlmP_cuduIWCh3qax3w_38eXx7coXlNYUwrVx-vL79s1A5Bro6iW4kmxolKaEpQQT4sV0EqVzFTsefEixhsAKiTVq-Jum4JNPu53GFxL_G8_IXHRJ79HglP-2404JRLT3DnsSHMgcW5GNwxuxISB_LK3SHbL6LtD9gbbOZ-lcDgjaYfENxHDrU3OT6S1e9u4wSWHkfiebL9ebS62L4tnvR0ivrp_T4ofny-uz7-Um2-XV-efNmUrmEmlyIFNJZocvOmA9VypxnCmleo7IXsBbT6D6AzjmlnBZWfQNIxLBaA5w56fFKfHvfvgf84YUz262OIw2An9HGujFROghc7k-0dJVoGUTPH_g4aCoNpk8MOjINUauDRKQkbf_oPe-DlM-TJ11jWAAZUhOEJt8DEG7Ot9cKMNh5pCvfShXvpQL32oj33Ilnf3e21s7dAHO7UuPvi0lBX8jfrmyDlEfJBltVyG_wFaMr4s</recordid><startdate>200603</startdate><enddate>200603</enddate><creator>Kasai, Y.J.</creator><creator>Urban, J.</creator><creator>Takahashi, C.</creator><creator>Hoshino, S.</creator><creator>Takahashi, K.</creator><creator>Inatani, J.</creator><creator>Shiotani, M.</creator><creator>Masuko, H.</creator><general>IEEE</general><general>Institute of Electrical and Electronics Engineers</general><general>The Institute of Electrical and Electronics Engineers, Inc. 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However, there are so far no published satellite measurements on the spatial and temporal variations of ozone isotopes in the stratosphere. Spectroscopic remote sensing methods can theoretically be used to observe ozone isotope fractionation on a global scale, but sufficient accuracy has not yet been achieved. A new generation of submillimeter-wave receivers employing sensitive superconductor-insulator-superconductor (SIS) detector technology will provide new opportunities for precise remote sensing measurements of ozone isotopes on a global scale. We have estimated the observation capabilities of two different SIS instruments, namely the space-station-borne Japanese Experimental Module/Sub-Millimeter-wave Limb Emission Sounder (JEM/SMILES) instrument, currently planned for launch in 2008, as well as the airborne Submillimeter wave Atmospheric Sounder/Airborne Submillimeter SIS Radiometer (SUMAS/ASUR) sensor. Measurements of the airborne sensor, conducted in 1996, are presented in order to demonstrate the detection of normal-O/sub 3/ and asymmetric-18-O/sub 3/ in the SMILES frequency bands. In the ideal case, JEM/SMILES has the capability to measure the ozone isotope enrichment (/spl delta//sup M/O/sub 3/) in the middle stratosphere with a precision of /spl sim/12/sup 0///sub 00/, /spl sim/11/sup 0///sub 00/, and /spl sim/9/sup 0///sub 00/, for asymmetric-18-O/sub 3/, symmetric-17-O/sub 3/, asymmetric-17-O/sub 3/, respectively, for a daily zonal mean product with resolution of 10/spl deg/ in latitude. The systematic error, including contributions of all instrumental and spectroscopic uncertainties, is estimated to be of the order of 100/sup 0///sub 00/ to 200/sup 0///sub 00/ and should be reduced by prelaunch laboratory measurements and in-flight calibrations. A remaining bias in the SMILES measurements will have to be quantified by dedicated validation campaigns. JEM/SMILES should then be capable to provide valuable information on the global distribution and seasonal variation of ozone isotope fractionation in the stratosphere. This new technology will allow us to shed new light on this still open issue in atmospheric sciences.</abstract><cop>New York, NY</cop><pub>IEEE</pub><doi>10.1109/TGRS.2005.861754</doi><tpages>18</tpages></addata></record> |
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subjects | Acoustic sensors Airborne sensing Applied geophysics Asymmetry Atmospheric measurements Atmospheric profiles retrieval Atmospheric sciences Atmospherics Carbon Chemical processes Earth sciences Earth, ocean, space Exact sciences and technology Fractionation Instruments Internal geophysics Isotopes limb sounder microwave spectroscopy Ozone Radiometry Remote sensing Spectroscopy Stratosphere stratospheric chemistry submillimeter wavelength superconducting receiver Terrestrial atmosphere |
title | Stratospheric ozone isotope enrichment studied by submillimeter wave heterodyne radiometry: the observation capabilities of SMILES |
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