A Cavity-Enhanced UV Absorption Instrument for High Precision, Fast Time Response Ozone Measurements

dc.contributor.authorHannun, Reem A.
dc.contributor.authorSwanson, Andrew K.
dc.contributor.authorBailey, Steven A.
dc.contributor.authorHanisco, Thomas F.
dc.contributor.authorBui, T. Paul
dc.contributor.authorBourgeois, Ilann
dc.contributor.authorPeischl, Jeff
dc.contributor.authorRyerson, Thomas B.
dc.date.accessioned2020-08-17T19:58:12Z
dc.date.available2020-08-17T19:58:12Z
dc.date.issued2020-07-22
dc.description.abstractThe NASA Rapid Ozone Experiment (ROZE) is a broadband cavity-enhanced UV absorption instrument for the detection of in situ ozone (O₃). ROZE uses an incoherent LED light source coupled to a high-finesse optical cavity to achieve an effective pathlength of ~ 104 m. Due to its high-sensitivity and small optical cell volume, ROZE demonstrates a 1σ precision of 80 pptv (0.1 s) and 31 pptv (1 s), as well as a 1/e response time of 50 ms. ROZE can be operated in a range of field environments, including low- and high-altitude research aircraft, and is particularly suited to O₃ vertical flux measurements using the eddy covariance technique. ROZE was successfully integrated aboard the NASA DC-8 aircraft during July–September 2019 and validated against a well-established chemiluminescence measurement of O₃. A flight within the marine boundary layer also demonstrated flux measurement capabilities, and we observed a mean O₃ deposition velocity of 0.029 ± 0.005 cm s⁻¹ to the ocean surface. The performance characteristics detailed below make ROZE a robust, versatile instrument for field measurements of O₃.en_US
dc.description.sponsorshipThis work was supported by the NASA Internal Research and Development (IRAD) program, the NASA Upper Atmosphere Research Program, and the NASA Tropospheric Chemistry Program. The aircraft flight opportunity was provided by the NASA/NOAA FIREX-AQ project and the NASA Student Airborne Research Program (SARP). We would like to acknowledge the DLH instrument team (Glenn Diskin, et al.) for the water vapor measurements used in the eddy covariance analysis. We would additionally like to thank Jason St. Clair and Glenn Wolfe for helpful comments on the manuscript.en_US
dc.description.urihttps://amt.copernicus.org/preprints/amt-2020-195/en_US
dc.format.extent20 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2m05n-ckp5
dc.identifier.citationHannun, Reem A.; Swanson, Andrew K.; Bailey, Steven A.; Hanisco, Thomas F.; Bui, T. Paul; Bourgeois, Ilann; Peischl, Jeff; Ryerson, Thomas B.; A Cavity-Enhanced UV Absorption Instrument for High Precision, Fast Time Response Ozone Measurements; Atmospheric Measurement Techniques (2020); https://amt.copernicus.org/preprints/amt-2020-195/en_US
dc.identifier.urihttps://doi.org/10.5194/amt-2020-195
dc.identifier.urihttp://hdl.handle.net/11603/19451
dc.language.isoen_USen_US
dc.publisherEGU Publicationsen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Physics Department Collection
dc.relation.ispartofUMBC Joint Center for Earth Systems Technology (JCET)
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsAttribution 4.0 International (CC BY 4.0)*
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/*
dc.titleA Cavity-Enhanced UV Absorption Instrument for High Precision, Fast Time Response Ozone Measurementsen_US
dc.typeTexten_US

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