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Solar cycle variability in middle atmospheric ozone over tropics.

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Title: Solar cycle variability in middle atmospheric ozone over tropics.
Authors: Fadnavis, S.1 (AUTHOR) Suvarna@tropmet.res.in, Beig, G.1 (AUTHOR)
Source: International Journal of Remote Sensing. Feb2010, Vol. 31 Issue 3, p565-573. 9p. 2 Graphs.
Subjects: Ozone, Ozonolysis, Chemosphere, Solar activity, Atmospheric chemistry, Mesosphere, Atmospheric ozone, Spherical astronomy, Solar oscillations, Symmetry (Biology), Regression analysis
Abstract: To investigate the effects of decadal solar variability in ozone, data obtained from the Halogen Occultation Experiment (HALOE) onboard Upper Atmospheric Research Satellite (UARS) during the period 1992-2004 have been analysed using a multifunctional regression model. Solar effects on ozone are analysed over the 0-30˚ N and 0-30˚ S belts. The solar effect on ozone is found to be significant in most of the stratosphere (2 ± 1.1 to 4 ± 1.6%/100 sfu). It is negligible in the lower mesosphere whereas it is of the order of 5%/100 sfu in the upper mesosphere. These observed results are in reasonable agreement with model simulations. Results indicate a hemispheric symmetry in the tropics. Results obtained in the present study are also compared with the results obtained by other workers. [ABSTRACT FROM AUTHOR]
Copyright of International Journal of Remote Sensing is the property of Taylor & Francis Ltd and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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Header DbId: egs
DbLabel: Engineering Source
An: 49143191
AccessLevel: 6
PubType: Academic Journal
PubTypeId: academicJournal
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  Label: Title
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  Data: Solar cycle variability in middle atmospheric ozone over tropics.
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  Data: <searchLink fieldCode="AR" term="%22Fadnavis%2C+S%2E%22">Fadnavis, S.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> Suvarna@tropmet.res.in</i><br /><searchLink fieldCode="AR" term="%22Beig%2C+G%2E%22">Beig, G.</searchLink><relatesTo>1</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22International+Journal+of+Remote+Sensing%22">International Journal of Remote Sensing</searchLink>. Feb2010, Vol. 31 Issue 3, p565-573. 9p. 2 Graphs.
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  Data: <searchLink fieldCode="DE" term="%22Ozone%22">Ozone</searchLink><br /><searchLink fieldCode="DE" term="%22Ozonolysis%22">Ozonolysis</searchLink><br /><searchLink fieldCode="DE" term="%22Chemosphere%22">Chemosphere</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+activity%22">Solar activity</searchLink><br /><searchLink fieldCode="DE" term="%22Atmospheric+chemistry%22">Atmospheric chemistry</searchLink><br /><searchLink fieldCode="DE" term="%22Mesosphere%22">Mesosphere</searchLink><br /><searchLink fieldCode="DE" term="%22Atmospheric+ozone%22">Atmospheric ozone</searchLink><br /><searchLink fieldCode="DE" term="%22Spherical+astronomy%22">Spherical astronomy</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+oscillations%22">Solar oscillations</searchLink><br /><searchLink fieldCode="DE" term="%22Symmetry+%28Biology%29%22">Symmetry (Biology)</searchLink><br /><searchLink fieldCode="DE" term="%22Regression+analysis%22">Regression analysis</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: To investigate the effects of decadal solar variability in ozone, data obtained from the Halogen Occultation Experiment (HALOE) onboard Upper Atmospheric Research Satellite (UARS) during the period 1992-2004 have been analysed using a multifunctional regression model. Solar effects on ozone are analysed over the 0-30˚ N and 0-30˚ S belts. The solar effect on ozone is found to be significant in most of the stratosphere (2 ± 1.1 to 4 ± 1.6%/100 sfu). It is negligible in the lower mesosphere whereas it is of the order of 5%/100 sfu in the upper mesosphere. These observed results are in reasonable agreement with model simulations. Results indicate a hemispheric symmetry in the tropics. Results obtained in the present study are also compared with the results obtained by other workers. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of International Journal of Remote Sensing is the property of Taylor & Francis Ltd and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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RecordInfo BibRecord:
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      – Type: doi
        Value: 10.1080/01431160902893535
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      – Code: eng
        Text: English
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      Pagination:
        PageCount: 9
        StartPage: 565
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      – SubjectFull: Ozone
        Type: general
      – SubjectFull: Ozonolysis
        Type: general
      – SubjectFull: Chemosphere
        Type: general
      – SubjectFull: Solar activity
        Type: general
      – SubjectFull: Atmospheric chemistry
        Type: general
      – SubjectFull: Mesosphere
        Type: general
      – SubjectFull: Atmospheric ozone
        Type: general
      – SubjectFull: Spherical astronomy
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      – SubjectFull: Solar oscillations
        Type: general
      – SubjectFull: Symmetry (Biology)
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      – SubjectFull: Regression analysis
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      – TitleFull: Solar cycle variability in middle atmospheric ozone over tropics.
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            NameFull: Fadnavis, S.
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            NameFull: Beig, G.
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              Text: Feb2010
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              Y: 2010
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