Show simple item record Brown, Daniel Parnell, Clare Deluca, E. E. Golub, Leon McMullen, Rebecca 2007-01-16T13:32:46Z 2007-01-16T13:32:46Z 2001-07-01
dc.identifier.citation Brown , D , Parnell , C , Deluca , E E , Golub , L & McMullen , R 2001 , ' The magnetic structure of a coronal X-ray bright point ' Solar Physics , vol 201 , no. 2 , pp. 305-321 . DOI: 10.1023/A:1017907406350 en
dc.identifier.issn 0038-0938
dc.identifier.other PURE: 71679
dc.identifier.other PURE UUID: e7a3ef2a-69a5-42fa-ad81-c463c61f394c
dc.identifier.other dspace: 2160/296
dc.identifier.other DSpace_20121128.csv: row: 232
dc.identifier.other Scopus: 0035600740
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.rights en
dc.title The magnetic structure of a coronal X-ray bright point en
dc.type /dk/atira/pure/researchoutput/researchoutputtypes/contributiontojournal/article en
dc.contributor.institution Department of Physics en
dc.contributor.institution Mathematics and Physics en
dc.description.status Peer reviewed en

Files in this item

Aside from theses and in the absence of a specific licence document on an item page, all works in Cadair are accessible under the CC BY-NC-ND Licence. AU theses and dissertations held on Cadair are made available for the purposes of private study and non-commercial research and brief extracts may be reproduced under fair dealing for the purpose of criticism or review. If you have any queries in relation to the re-use of material on Cadair, contact

This item appears in the following Collection(s)

Show simple item record

Search Cadair

Advanced Search