The long-term evolution of AR 7978: The scalings of the coronal plasma parameters with the mean photospheric magnetic field
We analyze the evolution of the fluxes observed in X-rays and correlate them with the magnetic flux density in active region (AR) NOAA 7978 from its birth throughout its decay, for five solar rotations. We use Solar and Heliospheric Observatory Michelson Doppler Imager (MDI) data, together with Yohk...
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2003
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v586_n1I_p579_VanDrielGesztelyi http://hdl.handle.net/20.500.12110/paper_0004637X_v586_n1I_p579_VanDrielGesztelyi |
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