Articles | Volume 15, issue 2
https://doi.org/10.5194/acp-15-829-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/acp-15-829-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Sunset–sunrise difference in solar occultation ozone measurements (SAGE II, HALOE, and ACE–FTS) and its relationship to tidal vertical winds
T. Sakazaki
CORRESPONDING AUTHOR
Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Japan
M. Shiotani
Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Japan
M. Suzuki
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan
D. Kinnison
National Center for Atmospheric Research, Boulder, USA
J. M. Zawodny
NASA Langley Research Center, Hampton, USA
M. McHugh
Global Atmospheric Technologies and Sciences, Newport News, USA
K. A. Walker
Department of Physics, University of Toronto, Toronto, Canada
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Cited
16 citations as recorded by crossref.
- Middle atmospheric ozone, nitrogen dioxide and nitrogen trioxide in 2002–2011: SD-WACCM simulations compared to GOMOS observations E. Kyrölä et al. 10.5194/acp-18-5001-2018
- Microwave radiometer observations of the ozone diurnal cycle and its short-term variability over Switzerland E. Sauvageat et al. 10.5194/acp-23-7321-2023
- Evaluation of the Ozone Fields in NASA’s MERRA-2 Reanalysis K. Wargan et al. 10.1175/JCLI-D-16-0699.1
- Evaluation of CESM1 (WACCM) free-running and specified dynamics atmospheric composition simulations using global multispecies satellite data records L. Froidevaux et al. 10.5194/acp-19-4783-2019
- Validation of SAGE III/ISS Solar Occultation Ozone Products With Correlative Satellite and Ground‐Based Measurements H. Wang et al. 10.1029/2020JD032430
- The impact of nonuniform sampling on stratospheric ozone trends derived from occultation instruments R. Damadeo et al. 10.5194/acp-18-535-2018
- SAGE III/ISS ozone and NO2 validation using diurnal scaling factors S. Strode et al. 10.5194/amt-15-6145-2022
- Subpolar Activation of Halogen Heterogeneous Chemistry in Austral Spring B. Zambri et al. 10.1029/2020GL090036
- Thermal tides in the middle atmosphere at mid-latitudes measured with a ground-based microwave radiometer W. Krochin et al. 10.5194/amt-17-5015-2024
- Model estimations of geophysical variability between satellite measurements of ozone profiles P. Sheese et al. 10.5194/amt-14-1425-2021
- Ground-based assessment of the bias and long-term stability of 14 limb and occultation ozone profile data records D. Hubert et al. 10.5194/amt-9-2497-2016
- Model-based climatology of diurnal variability in stratospheric ozone as a data analysis tool S. Frith et al. 10.5194/amt-13-2733-2020
- Ozone and temperature decadal solar-cycle responses, and their relation to diurnal variations in the stratosphere, mesosphere, and lower thermosphere, based on measurements from SABER on TIMED F. Huang & H. Mayr 10.5194/angeo-37-471-2019
- The Stratospheric Water and Ozone Satellite Homogenized (SWOOSH) database: a long-term database for climate studies S. Davis et al. 10.5194/essd-8-461-2016
- Three‐dimensional structures of tropical nonmigrating tides in a high‐vertical‐resolution general circulation model T. Sakazaki et al. 10.1002/2014JD022464
- Representation of solar tides in the stratosphere and lower mesosphere in state-of-the-art reanalyses and in satellite observations T. Sakazaki et al. 10.5194/acp-18-1437-2018
16 citations as recorded by crossref.
- Middle atmospheric ozone, nitrogen dioxide and nitrogen trioxide in 2002–2011: SD-WACCM simulations compared to GOMOS observations E. Kyrölä et al. 10.5194/acp-18-5001-2018
- Microwave radiometer observations of the ozone diurnal cycle and its short-term variability over Switzerland E. Sauvageat et al. 10.5194/acp-23-7321-2023
- Evaluation of the Ozone Fields in NASA’s MERRA-2 Reanalysis K. Wargan et al. 10.1175/JCLI-D-16-0699.1
- Evaluation of CESM1 (WACCM) free-running and specified dynamics atmospheric composition simulations using global multispecies satellite data records L. Froidevaux et al. 10.5194/acp-19-4783-2019
- Validation of SAGE III/ISS Solar Occultation Ozone Products With Correlative Satellite and Ground‐Based Measurements H. Wang et al. 10.1029/2020JD032430
- The impact of nonuniform sampling on stratospheric ozone trends derived from occultation instruments R. Damadeo et al. 10.5194/acp-18-535-2018
- SAGE III/ISS ozone and NO2 validation using diurnal scaling factors S. Strode et al. 10.5194/amt-15-6145-2022
- Subpolar Activation of Halogen Heterogeneous Chemistry in Austral Spring B. Zambri et al. 10.1029/2020GL090036
- Thermal tides in the middle atmosphere at mid-latitudes measured with a ground-based microwave radiometer W. Krochin et al. 10.5194/amt-17-5015-2024
- Model estimations of geophysical variability between satellite measurements of ozone profiles P. Sheese et al. 10.5194/amt-14-1425-2021
- Ground-based assessment of the bias and long-term stability of 14 limb and occultation ozone profile data records D. Hubert et al. 10.5194/amt-9-2497-2016
- Model-based climatology of diurnal variability in stratospheric ozone as a data analysis tool S. Frith et al. 10.5194/amt-13-2733-2020
- Ozone and temperature decadal solar-cycle responses, and their relation to diurnal variations in the stratosphere, mesosphere, and lower thermosphere, based on measurements from SABER on TIMED F. Huang & H. Mayr 10.5194/angeo-37-471-2019
- The Stratospheric Water and Ozone Satellite Homogenized (SWOOSH) database: a long-term database for climate studies S. Davis et al. 10.5194/essd-8-461-2016
- Three‐dimensional structures of tropical nonmigrating tides in a high‐vertical‐resolution general circulation model T. Sakazaki et al. 10.1002/2014JD022464
- Representation of solar tides in the stratosphere and lower mesosphere in state-of-the-art reanalyses and in satellite observations T. Sakazaki et al. 10.5194/acp-18-1437-2018
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Latest update: 13 Dec 2024
Short summary
The solar occultation measurements measure the atmosphere at sunrise (SR) and sunset (SS). It has been reported that there is a significant difference in the observed amount of stratospheric ozone between SR and SS. This study first revealed that this difference can be largely explained by diurnal variations in ozone, particularly those caused by vertical transport by the atmospheric tidal winds. Our results would be helpful for the construction of combined data sets from SR and SS profiles.
The solar occultation measurements measure the atmosphere at sunrise (SR) and sunset (SS). It...
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