An empirical 3D model of the large-scale coronal structure based on the distribution of H$\alpha$ filaments on the solar disk

Publisher： Edp Sciences

E-ISSN： 1432-0746|464|1|357-365

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.464, Iss.1, 2007-03, pp. : 357-365

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