Distribution of electric currents in sunspots from photosphere to corona

We present a study of two regular sunspots that exhibit nearly uniform twist from the photosphere to the corona. We derive the twist parameter in the corona and in the chromosphere by minimizing the difference between the extrapolated linear force-free field model field lines and the observed intens...

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Detalles Bibliográficos
Autores principales: Gosain, S., Démoulin, P., López Fuentes, M.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v793_n1_p_Gosain
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