The magnetic structure of a coronal X-ray bright point

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dc.contributor.author Golub, Leon
dc.contributor.author Brown, Daniel
dc.contributor.author DeLuca, Ed
dc.contributor.author McMullen, Rebecca
dc.contributor.author Parnell, Clare
dc.date.accessioned 2007-01-16T13:32:46Z
dc.date.available 2007-01-16T13:32:46Z
dc.date.issued 2001
dc.identifier.citation Golub , L , Brown , D , DeLuca , E , McMullen , R & Parnell , C 2001 , ' The magnetic structure of a coronal X-ray bright point ' Solar Physics , pp. 305-321 . , 10.1023/A:1017907406350 en
dc.identifier.other PURE: 71679
dc.identifier.other dspace: 2160/296
dc.identifier.uri http://hdl.handle.net/2160/296
dc.description Brown, D.S., Parnell, C.E., Deluca, E., McMullen, R. and Golub, L., 2001, The magnetic structure of a coronal X-ray bright point, Solar Physics, 201, 305-321. en
dc.description.abstract Abstract. X-ray bright points are small dynamic loop structures that are observed all over the solar corona. The high spatial and temporal resolution of the TRACE instrument allows bright points to be studied in much greater detail than previously possible. This paper focusses on a specifc bright point which occurred for about 20 hours on the 13-14th June 1998 and examines its dynamic structure in detail. This example suggests that the mechanisms that cause bright points to form and evolve are more complex than previously thought. In this case, reconnection probably plays a major part during the formation and brightening of the loop structure. However, later on the foot points rotate injecting twist into the bright point which may cause an instability to occur with dynamic results. en
dc.format.extent 17 en
dc.language.iso eng
dc.relation.ispartof Solar Physics en
dc.title The magnetic structure of a coronal X-ray bright point en
dc.type Text en
dc.type.publicationtype Article (Journal) en
dc.identifier.doi http://dx.doi.org/10.1023/A:1017907406350
dc.contributor.institution Institute of Mathematics & Physics (ADT) en
dc.contributor.institution Mathematics and Physics en
dc.description.status Peer reviewed en


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