| dc.date.accessioned | 2013-03-12T08:26:12Z | |
| dc.date.available | 2013-03-12T08:26:12Z | |
| dc.date.issued | 2012 | en_US |
| dc.date.submitted | 2012-05-07 | en_US |
| dc.identifier.citation | Hole, Ida Benedikte Amlie. The Inverse-C shape of the {\Caiinm} Spectral Line. Masteroppgave, University of Oslo, 2012 | en_US |
| dc.identifier.uri | http://hdl.handle.net/10852/10928 | |
| dc.description.abstract | The inverse-C shape of the bisector from the chromospheric Ca triplet spectral lines is a little understood phenomena. This spectral signature can give valuble information about the chromosphere, which is the least understood atmospheric layer of the Sun. Principal Component Analysis is applied to high spatial and spectral resolution observations obtained at the Swedish 1-m Solar Telescope to study which spectral line profiles that contribute to this inverse-C shape. | eng |
| dc.language.iso | nob | en_US |
| dc.title | The Inverse-C shape of the {\Caiinm} Spectral Line | en_US |
| dc.type | Master thesis | en_US |
| dc.date.updated | 2012-09-15 | en_US |
| dc.creator.author | Hole, Ida Benedikte Amlie | 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=Hole, Ida Benedikte Amlie&rft.title=The Inverse-C shape of the {\Caiinm} Spectral Line&rft.inst=University of Oslo&rft.date=2012&rft.degree=Masteroppgave | en_US |
| dc.identifier.urn | URN:NBN:no-31607 | en_US |
| dc.type.document | Masteroppgave | en_US |
| dc.identifier.duo | 158435 | en_US |
| dc.contributor.supervisor | Mats Carlsson | en_US |
| dc.identifier.bibsys | 122629663 | en_US |
| dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/10928/1/main.pdf | |