| dc.date.accessioned | 2018-02-16T16:34:45Z | |
| dc.date.available | 2018-08-31T22:31:24Z | |
| dc.date.created | 2017-10-14T11:42:53Z | |
| dc.date.issued | 2017 | |
| dc.identifier.citation | Zirker, Jack B. Engvold, Oddbjørn . Why is the Sun's corona so hot? Why are prominences so cool?. Physics today. 2017, 70(8), 36-43 | |
| dc.identifier.uri | http://hdl.handle.net/10852/60191 | |
| dc.description.abstract | © 2017 American Institute of Physics. | en_US |
| dc.language | EN | |
| dc.language.iso | en | en_US |
| dc.title | Why is the Sun's corona so hot? Why are prominences so cool? | en_US |
| dc.type | Journal article | en_US |
| dc.creator.author | Zirker, Jack B. | |
| dc.creator.author | Engvold, Oddbjørn | |
| cristin.unitcode | 185,15,3,0 | |
| cristin.unitname | Institutt for teoretisk astrofysikk | |
| cristin.ispublished | true | |
| cristin.fulltext | original | |
| cristin.qualitycode | 1 | |
| dc.identifier.cristin | 1504623 | |
| dc.identifier.bibliographiccitation | info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physics today&rft.volume=70&rft.spage=36&rft.date=2017 | |
| dc.identifier.jtitle | Physics today | |
| dc.identifier.volume | 70 | |
| dc.identifier.issue | 8 | |
| dc.identifier.startpage | 36 | |
| dc.identifier.endpage | 43 | |
| dc.identifier.doi | http://dx.doi.org/10.1063/PT.3.3659 | |
| dc.identifier.urn | URN:NBN:no-62840 | |
| dc.type.document | Tidsskriftartikkel | en_US |
| dc.type.peerreviewed | Peer reviewed | |
| dc.source.issn | 0031-9228 | |
| dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/60191/1/pt.3.3659.pdf | |
| dc.type.version | PublishedVersion | |