Magnetic Topology of Active Regions and Coronal Holes: Implications for Coronal Outflows and the Solar Wind
During 2-18 January 2008 a pair of low-latitude opposite-polarity coronal holes (CHs) were observed on the Sun with two active regions (ARs) and the heliospheric plasma sheet located between them. We use the Hinode/EUV Imaging Spectrometer (EIS) to locate AR-related outflows and measure their veloci...
Guardado en:
| Autores principales: | Mandrini, Cristina Hemilse, Stenborg, Guillermo Adrián |
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| Publicado: |
2012
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| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v281_n1_p237_vanDrielGesztelyi http://hdl.handle.net/20.500.12110/paper_00380938_v281_n1_p237_vanDrielGesztelyi |
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