Helium line formation and abundance during a C-class flare

During a coordinated campaign that took place in 2001 May, a C-class flare was observed both with SOHO instruments and with the Dunn Solar Telescope of the National Solar Observatory at Sacramento Peak. In two previous papers we described the observations and discussed some dynamical aspects of the...

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Autores principales: Andretta, V., Mauas, P.J.D., Falchi, A., Teriaca, L.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v681_n1_p650_Andretta
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