globalchange  > 影响、适应和脆弱性
DOI: 10.1002/jgrd.50445
论文题名:
Satellite observations of ozone in the upper mesosphere
作者: Smith A.K.; Harvey V.L.; Mlynczak M.G.; Funke B.; García-Comas M.; Hervig M.; Kaufmann M.; Kyrölä E.; Lõpez-Puertas M.; McDade I.; Randall C.E.; Russell J.M.; Sheese P.E.; Shiotani M.; Skinner W.R.; Suzuki M.; Walker K.A.
刊名: Journal of Geophysical Research Atmospheres
ISSN: 21698996
出版年: 2013
卷: 118, 期:11
起始页码: 5803
结束页码: 5821
语种: 英语
英文关键词: mesosphere ; ozone ; SABER
Scopus关键词: Atmospheric chemistry ; Experiments ; Infrared imaging ; Instruments ; Michelson interferometers ; Atmospheric chemistry experiment ; Fourier transform spectrometers ; Global ozone monitoring by occultation of stars ; Halogen occultation experiments ; mesosphere ; Michelson interferometer for passive atmospheric soundings ; SABER ; Sounding of the atmosphere using broadband emission radiometry ; Ozone ; atmospheric chemistry ; data set ; mesosphere ; mixing ratio ; ozone ; radiometer ; satellite imagery ; vertical profile
英文摘要: Ozone profiles in the upper mesosphere (70-100 km) retrieved from nine instruments are compared. Ozone from the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument is used as the basis of comparison. Other measurements are from the Halogen Occultation Experiment, the High Resolution Doppler Imager, the Michelson Interferometer for Passive Atmospheric Sounding, the Global Ozone Monitoring by Occultation of Stars, the Atmospheric Chemistry Experiment - Fourier Transform Spectrometer, the Solar Occultation For Ice Experiment, the Optical Spectrograph and InfraRed Imaging System, and the Superconducting Submillimeter-Wave Limb-Emission Sounder. Comparisons of each data set with SABER using coincident profiles indicate agreement in the basic vertical profile of ozone but also some systematic differences in daytime ozone. Ozone from the SABER 9.6 μm channel is higher than the other measurements over the altitude range 60-80 km by 20-50%. Nighttime comparisons indicate better relative agreement (<10% difference). Taking all the data, not limited to coincidences, shows the global and seasonal distributions of ozone in the upper mesosphere from each instrument. The average maximum in ozone mixing ratio is around 90-92 km during daytime and 95 km at night. There is a maximum in ozone density at night (∼90 km) and during some hours of the day. The latitude structure of ozone has appreciable variations with season, particularly in the tropical upper mesosphere. The basic latitude-altitude structure of ozone depends on local time, even when the analysis is restricted to day-only observations. © 2013. American Geophysical Union. All Rights Reserved.
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/63685
Appears in Collections:影响、适应和脆弱性
气候减缓与适应

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作者单位: Atmospheric Chemistry Division, National Center for Atmospheric Research, PO Box 3000, Boulder, CO 80307, United States; Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, United States; NASA Langley Research Center, Hampton, VA, United States; Instituto de Astrofisica de Andalucía, Granada, Spain; GATS, Inc., Driggs, ID, United States; Forschungszentrum Jülich, Jülich, Germany; Finnish Meteorological Institute, Helsinki, Finland; Department of Earth and Space Science and Engineering, York University, Toronto, ON, Canada; Department of Atmospheric and Oceanic Sciences, University of Colorado Boulder, Boulder, CO, United States; Center for Atmospheric Sciences, Hampton University, Hampton, VA, United States; Department of Physics, University of Toronto, Toronto, ON, Canada; Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Japan; Space Physics Research Laboratory, University of Michigan, Ann Arbor, MI, United States; Japan Aerospace Exploration Agency, Sagamihara, Japan

Recommended Citation:
Smith A.K.,Harvey V.L.,Mlynczak M.G.,et al. Satellite observations of ozone in the upper mesosphere[J]. Journal of Geophysical Research Atmospheres,2013-01-01,118(11)
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