The 3D Geometry of Active Region Upflows Deduced from Their Limb-to-Limb Evolution

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We analyze the evolution of coronal plasma upflows from the edges of AR 10978, which has the best limb-to-limb data coverage with Hinode's EUV Imaging Spectrometer (EIS). We find that the observed evolution is largely due to the solar rotation progressively changing the viewpoint of nearly stat...

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Detalles Bibliográficos
Autores principales: Démoulin, P., Baker, D., Mandrini, C.H., van Driel-Gesztelyi, L.
Formato: JOUR
Materias:
Active regions, magnetic fields
Active regions, velocity field
Corona, active
Spectral line, broadening
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00380938_v283_n2_p341_Demoulin
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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