Apparent and Intrinsic Evolution of Active Region Upflows

We analyze the evolution of Fe xii coronal plasma upflows from the edges of ten active regions (ARs) as they cross the solar disk using the Hinode Extreme Ultraviolet Imaging Spectrometer (EIS) to do this. Confirming the results of Démoulin et al. (Sol. Phys.283, 341, 2013), we find that for each AR...

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Detalles Bibliográficos
Publicado:	2017
Materias:	Active regions, magnetic fields Active regions, velocity field
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v292_n4_p_Baker http://hdl.handle.net/20.500.12110/paper_00380938_v292_n4_p_Baker
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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