Characterization of intensity variations along Fe XIV coronal loops - a case study
We discuss a method, and corresponding results, to analyze the dynamics of localized small-scale coronal (post-flare) loops observed with the MICA (Mirror Coronagraph for Argentina) telescope in the well-known green coronal line at 530.3 nm. In particular, we designed a procedure to measure intensit...
Guardado en:
| Publicado: |
2004
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v222_n2_p229_Costa http://hdl.handle.net/20.500.12110/paper_00380938_v222_n2_p229_Costa |
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