Articles | Volume 15, issue 2
Atmos. Chem. Phys., 15, 829–843, 2015
https://doi.org/10.5194/acp-15-829-2015
Atmos. Chem. Phys., 15, 829–843, 2015
https://doi.org/10.5194/acp-15-829-2015
Research article
23 Jan 2015
Research article | 23 Jan 2015

Sunset–sunrise difference in solar occultation ozone measurements (SAGE II, HALOE, and ACE–FTS) and its relationship to tidal vertical winds

T. Sakazaki et al.

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Cited articles

Beaver, G. M., Gordley, L., and Russell III, J. M.: Halogen Occultation Experiment (HALOE) altitude registration of atmospheric profile measurements: lessons learned and improvements made during the data validation phase, Proc. SPIE 2266, P. Soc. Photo-Opt. Ins., 266–280, https://doi.org/10.1117/12.187564, 1994.
Boone, C., D., Nassar, R., Walker, K. A., Rochon, Y., McLeod, S. D., Rinsland, C. P., and Bernath, P. F.: retrievals for the atmospheric chemistry experiment Fourier-transform spectrometer, Appl. Optics, 44, 7218–7231, 2005.
Damadeo, R. P., Zawodny, J. M., Thomason, L. W., and Iyer, N.: SAGE version 7.0 algorithm: application to SAGE II, Atmos. Meas. Tech., 6, 3539–3561, https://doi.org/10.5194/amt-6-3539-2013, 2013.
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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.
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