| dc.date.accessioned | 2013-03-12T08:25:30Z | |
| dc.date.available | 2013-03-12T08:25:30Z | |
| dc.date.issued | 2003 | en_US |
| dc.date.submitted | 2003-02-24 | en_US |
| dc.identifier.citation | Karlsen, Karl Niklas. An observational analysis of the solar chromospheric continuum intensity. Hovedoppgave, University of Oslo, 2003 | en_US |
| dc.identifier.uri | http://hdl.handle.net/10852/10948 | |
| dc.description.abstract | The thesis examines the relation between
the magnetic field as measured by MDI and
the continuum intensity at four different
wavelengths (1319, 1199, 1037 and 910Å) as
measured by SUMER. A method for copointing
the instruments is developed, and the correlation
between several quantites (e.g. intensity oscillations
and magnetic field strength) are analysed.
The results indicate that there is some kind of
coupling between the magnetic field and the dynamics
of the solar chromosphere, and the results are of
very good quality, mainly because of the copointing
method and the resolutions of the instruments. | nor |
| dc.language.iso | eng | en_US |
| dc.title | An observational analysis of the solar chromospheric continuum intensity | en_US |
| dc.type | Master thesis | en_US |
| dc.date.updated | 2003-08-14 | en_US |
| dc.creator.author | Karlsen, Karl Niklas | en_US |
| dc.subject.nsi | VDP::438 | en_US |
| dc.identifier.bibliographiccitation | info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&rft.au=Karlsen, Karl Niklas&rft.title=An observational analysis of the solar chromospheric continuum intensity&rft.inst=University of Oslo&rft.date=2003&rft.degree=Hovedoppgave | en_US |
| dc.identifier.urn | URN:NBN:no-5263 | en_US |
| dc.type.document | Hovedoppgave | en_US |
| dc.identifier.duo | 8987 | en_US |
| dc.contributor.supervisor | Mats Carlsson | en_US |
| dc.identifier.bibsys | 030557836 | en_US |
| dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/10948/1/karlsen.pdf | |