Outflows at the edges of active regions: Contribution to solar wind formation?
The formation of the slow solar wind has been debated for many years. In this Letter we show evidence of persistent outflow at the edges of an active region as measured by the EUV Imaging Spectrometer on board Hinode. The Doppler velocity ranged between 20 and 50 km s -1 and was consistent with a st...
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2008
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v676_n2PART2_pL147_Harra http://hdl.handle.net/20.500.12110/paper_0004637X_v676_n2PART2_pL147_Harra |
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