Magnetic and velocity properties of G-band bright points around a pore

Rangarajan, K. E; Sankarasubramanian, K; Nagaraju, K

Home
→
IIAP Publications
→
IIAP Publications
→
View Item

dc.contributor.author	Rangarajan, K. E
dc.contributor.author	Sankarasubramanian, K
dc.contributor.author	Nagaraju, K
dc.date.accessioned	2009-07-23T14:39:13Z
dc.date.available	2009-07-23T14:39:13Z
dc.date.issued	2009-06
dc.identifier.citation	Svetlana 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 - 258	en
dc.identifier.isbn	978-1-58381-690-5
dc.identifier.uri	http://hdl.handle.net/2248/4670
dc.description	Restricted Access
dc.description.abstract	Physical 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.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.ispartofseries	ASP Conference Series; Vol. 405
dc.relation.uri	http://adsabs.harvard.edu/abs/2009ASPC..405..255R	en
dc.relation.uri	http://aspbooks.org/custom/publications/paper/405-0255.html	en
dc.rights	© Astronomical Society of the Pacific	en
dc.subject	Magnetic Properties	en
dc.subject	Velocity Properties	en
dc.subject	G-Band Bright Points	en
dc.subject	GBPs	en
dc.subject	The Magnetic Field	en
dc.subject	Spatial Resolution	en
dc.title	Magnetic and velocity properties of G-band bright points around a pore	en
dc.type	Article	en