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Please use this identifier to cite or link to this item: http://paper.sci.ui.ac.id/jspui/handle/2808.28/67
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dc.contributor.authorBachtiar, Alhaji Akbar-
dc.contributor.authorRiminarsih, D.-
dc.contributor.authorSatria, Yudi-
dc.date.accessioned2016-02-27T08:43:25Z-
dc.date.available2016-02-27T08:43:25Z-
dc.date.issued2014-02-
dc.identifier.issn0972-0871-
dc.identifier.urihttp://paper.sci.ui.ac.id/jspui/handle/2808.28/67-
dc.description.abstractInthiswork,we revisited the QuasiPAS flow. This flow was originally proposed by Bachtiar [1]. He proposed this flow in order to provide more evidence on the existence of planar velocity dynamos. According to Bachtiar [1], there is no dynamo using the planarized version of QuasiPAS, but he found some new dynamos in the partly-planarized one. Using various parameters, we show that the planarization of poloidal part is more important than toroidal part. Our results show that the magnetic field’s profile improves when we decrease the portion of planarized-toroidal part. We also calculate the helicity of QuasiPAS flow and compare it with the original PAS.en_US
dc.language.isoen_USen_US
dc.publisherPushpa Publishing Houseen_US
dc.relation.ispartofseriesVolume 85;Issue 1-
dc.sourceFar East Journal of Mathematical Sciences (FJMS) Volume 85, Issue 1, Pages 87 - 97 (February 2014)en_US
dc.source.urihttp://www.pphmj.com/abstract/8229.htmen_US
dc.subjectEarth’s dynamoen_US
dc.subjectQuasiPASen_US
dc.subjectmagnetic fieldsen_US
dc.subjecthelicityen_US
dc.titleA REVIEW ON QuasiPAS FLOWen_US
dc.typeArticleen_US
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