Journal cover Journal topic
Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
Journal topic

Journal metrics

Journal metrics

  • IF value: 5.668 IF 5.668
  • IF 5-year value: 6.201 IF 5-year
    6.201
  • CiteScore value: 6.13 CiteScore
    6.13
  • SNIP value: 1.633 SNIP 1.633
  • IPP value: 5.91 IPP 5.91
  • SJR value: 2.938 SJR 2.938
  • Scimago H <br class='hide-on-tablet hide-on-mobile'>index value: 174 Scimago H
    index 174
  • h5-index value: 87 h5-index 87
Volume 15, issue 2
Atmos. Chem. Phys., 15, 829-843, 2015
https://doi.org/10.5194/acp-15-829-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
Atmos. Chem. Phys., 15, 829-843, 2015
https://doi.org/10.5194/acp-15-829-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

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.
Viewed  
Total article views: 1,785 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,055 650 80 1,785 54 53
  • HTML: 1,055
  • PDF: 650
  • XML: 80
  • Total: 1,785
  • BibTeX: 54
  • EndNote: 53
Views and downloads (calculated since 18 Jun 2014)
Cumulative views and downloads (calculated since 18 Jun 2014)
Cited  
Saved (final revised paper)  
Saved (discussion paper)  
Discussed (final revised paper)  
No discussed metrics found.
Discussed (discussion paper)  
No discussed metrics found.
Latest update: 26 Jun 2019
Publications Copernicus
Download
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...
Citation