Can the Superposition of Evaporative Flows Explain Broad Fe XXI Profiles during Solar Flares?
Journal article; PublishedVersion; Peer reviewed
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Year
2019Permanent link
http://urn.nb.no/CRIStin
1736218Metadata
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- Institutt for teoretisk astrofysikk [1306]
- CRIStin høstingsarkiv [31446]