Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/371
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dc.contributor.authorLal, M.
dc.date.accessioned2015-09-10T06:12:48Z
dc.date.accessioned2021-02-12T09:28:30Z-
dc.date.available2015-09-10T06:12:48Z
dc.date.available2021-02-12T09:28:30Z-
dc.date.issued2007
dc.identifier.citationBulletin of Astronomical Society of India, v.35, p.569-574, 2007en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/371-
dc.description.abstractWe have studied the influence of geomagnetic storms on the total ozone variability over equatorial and polar latitude region. Total Ozone Mapping Spectrometer (TOMS) and METEOR- 3 satellite have provided the long duration ozone variability from polar to equatorial latitude region. In the present study we have considered only severe and strong geomagnetic storm events between 2000 and 2005. The polar region shows an increase in the total ozone column abundance after the onset of geomagnetic storm. The equatorial region shows the increase in ozone abundance before as well as after the onset of severe magnetic storm. The increase in the total ozone column density is localized over the Pacific ocean. Solar flares could be the cause for the increase in ozone column density before the onset of geomagnetic storms.en_US
dc.language.isoenen_US
dc.subjectOzoneen_US
dc.subjectGeomagnetic stormsen_US
dc.subjectStratosphereen_US
dc.subjectTOMS satelliteen_US
dc.subjectMETEOR 3 satelliteen_US
dc.titleStudy of ozone variability at equatorial latitude during severe geomagnetic stormen_US
dc.typeArticleen_US
dc.identifier.accession090864
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