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<article xlink="http://www.w3.org/1999/xlink" dtd-version="1.0" article-type="general-sciences" lang="en"><front><journal-meta><journal-id journal-id-type="publisher">IJCRR</journal-id><journal-id journal-id-type="nlm-ta">I Journ Cur Res Re</journal-id><journal-title-group><journal-title>International Journal of Current Research and Review</journal-title><abbrev-journal-title abbrev-type="pubmed">I Journ Cur Res Re</abbrev-journal-title></journal-title-group><issn pub-type="ppub">2231-2196</issn><issn pub-type="opub">0975-5241</issn><publisher><publisher-name>Radiance Research Academy</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">1847</article-id><article-id pub-id-type="doi"/><article-id pub-id-type="doi-url"/><article-categories><subj-group subj-group-type="heading"><subject>General Sciences</subject></subj-group></article-categories><title-group><article-title>GEOMAGNETIC STORMS ASSOCIATED WITH IV-RADIO BURSTS AND THEIR RELATION WITH SOLAR AND INTERPLANETARY PARAMETERS&#13;
</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>.L.Verma</surname><given-names>P</given-names></name></contrib></contrib-group><pub-date pub-type="ppub"><day>25</day><month>04</month><year>2012</year></pub-date><volume/><issue/><fpage>77</fpage><lpage>84</lpage><permissions><copyright-statement>This article is copyright of Popeye Publishing, 2009</copyright-statement><copyright-year>2009</copyright-year><license license-type="open-access" href="http://creativecommons.org/licenses/by/4.0/"><license-p>This is an open-access article distributed under the terms of the Creative Commons Attribution (CC BY 4.0) Licence. You may share and adapt the material, but must give appropriate credit to the source, provide a link to the licence, and indicate if changes were made.</license-p></license></permissions><abstract><p>I have studied geomagnetic storms (Dst ?-75nT), associated with Type IV radio bursts, observed during the period 1997 to 2007 with solar and interplanetary parameters. We have observed 33 geomagnetic storms associated with type IV radio bursts, out of which most of the geomagnetic storms (85.00%) are intense or sever geomagnetic storms. All the geomagnetic storms are found to be associated with halo and partial halo coronal mass ejections (CMEs).The association rates of halo and partial halo CMEs are 27 (81.82%) and 06 (18.18%) respectively .All the type IV radio bursts associated geomagnetic storms are found to be associated with X-ray solar flares of different categories .The association rates of geomagnetic storms with different types of flare related CMEs are found 08 (24.24)% X class flare&#13;
related CMEs,15 ( 45.46% ) M class flare related CMEs ,08 (24.24 )% C class flare related CMEs and 02(6.06)% B class flare related CMEs. Some of the type IV radio bursts associated geomagnetic storms are found to be associated with magnetic clouds 13 (39.39 %).Majority of the geomagnetic storms are found to be related with interplanetary shocks 31 (93.94) .We have inferred that geomagnetic storms are closely related to interplanetary magnetic fields. We have determined positive co-relation with correlation coefficient 0.70 between magnitude of geomagnetic storms and maximum value of IMF and 0.77 between magnitude of geomagnetic storms and magnitude of maximum value of southward component of interplanetary magnetic fields (IMF Bz).&#13;
</p></abstract><kwd-group><kwd>Coronal mass ejections</kwd><kwd> X-ray solar flares</kwd><kwd> radio bursts</kwd><kwd> solar wind plasma parameters and geomagnetic storms.</kwd></kwd-group></article-meta></front></article>
