Adaptive Visualisierung koronaler Löcher

dc.contributor.author	Jähne, Sebastian	de
dc.date.accessioned	2012-12-21	de
dc.date.accessioned	2016-03-31T08:00:07Z
dc.date.available	2012-12-21	de
dc.date.available	2016-03-31T08:00:07Z
dc.date.issued	2012	de
dc.description.abstract	Coronal holes are structures on the photosphere of the sun. They are in close relation to so-called geomagnetic storms, which have the potential of harming electronic devices in space and even on Earth. We present a method for extracting the coronal holes from magnetic field data of the Sun in an adaptive refinement manner. In contrast to previous methods our algorithm produces vector graphics representation instead of a texture which would show coarsely approximated coronal holes only. It takes advantage of the fact that the magnetic field of the Sun can be topologically divided into two parts which define the coronal hole boundaries.	en
dc.identifier.other	377528978	de
dc.identifier.uri	http://nbn-resolving.de/urn:nbn:de:bsz:93-opus-80401	de
dc.identifier.uri	http://elib.uni-stuttgart.de/handle/11682/3008
dc.identifier.uri	http://dx.doi.org/10.18419/opus-2991
dc.language.iso	en	de
dc.rights	info:eu-repo/semantics/openAccess	de
dc.subject.ddc	004	de
dc.title	Adaptive Visualisierung koronaler Löcher	en
dc.title.alternative	Adaptive visualization of coronal holes	en
dc.type	StudyThesis	de
ubs.fakultaet	Fakultät Informatik, Elektrotechnik und Informationstechnik	de
ubs.institut	Institut für Visualisierung und Interaktive Systeme	de
ubs.opusid	8040	de
ubs.publikation.typ	Studienarbeit	de

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