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...
Guardado en:
Autores principales: | Gosain, S., Démoulin, P., López Fuentes, M. |
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Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v793_n1_p_Gosain |
Aporte de: |
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