Zur Kurzanzeige

dc.contributor.authorMikurda, Katarzyna
dc.date.accessioned2010-10-12T18:25:31Z
dc.date.available2010-10-12T18:25:31Z
dc.date.issued2006
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0001-30FA-3
dc.description.abstractPhotospheric bright points are proxies for small-scale magnetic flux concentrations.These magnetic elements are thought to be the building blocks of the solar magnetic field and are important to understand many physical processes on the Sun, e.g. the variability of the solar irradiance.Because of their small size (100-200 km in diameter) the observations of photospheric bright points put special requirements on the seeing conditions, instrumental setup and post-processing techniques ...
dc.format.extent105 S.
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherUniv. Freiburg (Breisgau)
dc.rights.urihttp://e-docs.geo-leo.de/rights
dc.subject.ddc523
dc.subject.gokTGC 800
dc.subject.gokTGC 745
dc.titleHigh resolution spectroscopy of photospheric bright points
dc.typemonograph
dc.subject.gokverbalMagnetfelder {Astronomie: Sonne}
dc.subject.gokverbalPhotosphäre {Astronomie: Sonne}
dc.identifier.doi10.23689/fidgeo-114
dc.identifier.ppn517850184
dc.identifier.urnurn:nbn:de:bsz:25-opus-24594
dc.type.versionpublishedVersion
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


Dateien zu dieser Ressource

Thumbnail

Das Dokument erscheint in:

Zur Kurzanzeige