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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4670
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dc.contributor.authorRangarajan, K. E-
dc.contributor.authorSankarasubramanian, K-
dc.contributor.authorNagaraju, K-
dc.date.accessioned2009-07-23T14:39:13Z-
dc.date.available2009-07-23T14:39:13Z-
dc.date.issued2009-06-
dc.identifier.citationSvetlana V. Berdyugina, K. N. Nagendra, and Renzo Ramelli., eds., Solar Polarization 5: In Honor of Jan Stenflo ASP Conference Series, Vol. 405, Proceedings of the Conference held 17 - 21 September, 2007 at Centro Stefano Franscini-Monte Veritá, Ascona, Switzerland., pp. 255 - 258en
dc.identifier.isbn978-1-58381-690-5-
dc.identifier.urihttp://hdl.handle.net/2248/4670-
dc.descriptionRestricted Access-
dc.description.abstractPhysical properties of G-band bright points (GBPs) surrounding a pore are studied using observations spanning from photosphere to chromosphere. The magnetic field strengths obtained in these bright points are of the order of 1.2 kG. These GBPs show very little linear polarization and the magnetic field lines are vertical. The observed GBPs show a fill-fraction between 20 to 40%, revealing that they are smaller than the achieved spatial resolution of 0.2 arcsec. The observed GBPs harbor accelerated downflows.en
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.ispartofseriesASP Conference Series; Vol. 405-
dc.relation.urihttp://adsabs.harvard.edu/abs/2009ASPC..405..255Ren
dc.relation.urihttp://aspbooks.org/custom/publications/paper/405-0255.htmlen
dc.rights© Astronomical Society of the Pacificen
dc.subjectMagnetic Propertiesen
dc.subjectVelocity Propertiesen
dc.subjectG-Band Bright Pointsen
dc.subjectGBPsen
dc.subjectThe Magnetic Fielden
dc.subjectSpatial Resolutionen
dc.titleMagnetic and velocity properties of G-band bright points around a poreen
dc.typeArticleen
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