Show simple item record

dc.contributor.authorHood, L. L.
dc.contributor.authorZhou, S.
dc.date.accessioned2017-06-07T20:05:23Z
dc.date.available2017-06-07T20:05:23Z
dc.date.issued1998-02-20
dc.identifier.citationStratospheric effects of 27-day solar ultraviolet variations: An analysis of UARS MLS ozone and temperature data 1998, 103 (D3):3629 Journal of Geophysical Research: Atmospheresen
dc.identifier.issn01480227
dc.identifier.doi10.1029/97JD02849
dc.identifier.urihttp://hdl.handle.net/10150/624009
dc.description.abstractThe characteristics of upper stratospheric ozone and temperature responses at low latitudes to short-term solar ultraviolet variations are studied by using 1000 days of UARS microwave limb sounder (MLS) and solar stellar irradiance comparison experiment data. Consistent with previous analyses of Nimbus 7 solar backscattered ultraviolet (SBUV) data, the high-pass-filtered solar flux in the 200-to 205-nm interval is most strongly correlated with MLS ozone measurements at tropical latitudes near 4 hPa with a sensitivity of about 0.4% for each 1% change in the solar flux. Reproducibility tests, power spectral, and coherency estimates support the reality of the observed ozone response at this level. The MLS solar UV/ozone response is significantly reduced at levels above ∼2 hPa as compared to earlier results based on SBUV data. This reduction appears to be a consequence of the ozone diurnal cycle at high altitudes combined with the necessary inclusion of nighttime records in calculating the MLS ozone zonal averages. Some evidence is obtained for an MLS solar UV/temperature response near the stratopause, but coherency tests are negative. Future analyses of independent data records having similar local time coverage as that of Nimbus 7 SBUV are needed to establish more definitively whether any significant change in the upper stratospheric UV response has occurred.
dc.description.sponsorshipSupported at the University of Arizona by NASA grant NAG53777 and at NOAA/NCEP by the NASA UARS program.en
dc.language.isoenen
dc.publisherAMER GEOPHYSICAL UNIONen
dc.relation.urlhttp://doi.wiley.com/10.1029/97JD02849en
dc.rightsCopyright 1998 by the American Geophysical Union.en
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.titleStratospheric effects of 27-day solar ultraviolet variations: An analysis of UARS MLS ozone and temperature dataen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Lunar & Planetary Laben
dc.identifier.journalJournal of Geophysical Research: Atmospheresen
dc.description.note6 month embargo; First published: 1 February 1998en
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
refterms.dateFOA1998-08-01T00:00:00Z
html.description.abstractThe characteristics of upper stratospheric ozone and temperature responses at low latitudes to short-term solar ultraviolet variations are studied by using 1000 days of UARS microwave limb sounder (MLS) and solar stellar irradiance comparison experiment data. Consistent with previous analyses of Nimbus 7 solar backscattered ultraviolet (SBUV) data, the high-pass-filtered solar flux in the 200-to 205-nm interval is most strongly correlated with MLS ozone measurements at tropical latitudes near 4 hPa with a sensitivity of about 0.4% for each 1% change in the solar flux. Reproducibility tests, power spectral, and coherency estimates support the reality of the observed ozone response at this level. The MLS solar UV/ozone response is significantly reduced at levels above ∼2 hPa as compared to earlier results based on SBUV data. This reduction appears to be a consequence of the ozone diurnal cycle at high altitudes combined with the necessary inclusion of nighttime records in calculating the MLS ozone zonal averages. Some evidence is obtained for an MLS solar UV/temperature response near the stratopause, but coherency tests are negative. Future analyses of independent data records having similar local time coverage as that of Nimbus 7 SBUV are needed to establish more definitively whether any significant change in the upper stratospheric UV response has occurred.


Files in this item

Thumbnail
Name:
Hood_et_al-1998-Journal_of_Geo ...
Size:
1.037Mb
Format:
PDF
Description:
Final Published Version

This item appears in the following Collection(s)

Show simple item record