Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..359w&link_type=abstract
Acta Astrophys. Sin., Vol. 15, No. 4, p. 359 - 364
Astronomy and Astrophysics
Astrophysics
Solar Corona: Magnetic Fields, Interplanetary Magnetic Field: Structure, Solar Magnetic Fields: Structure
Scientific paper
The authors calculated the global coronal (at 2.5 Rsun) magnetic field of Carrington rotations 1733 - 1742 using the boundary element method (BEM) under the linear force-free field model, based on photospheric magnetic field observations. The results are compared with those using the multiple expansion method under the potential field model. The two approaches indicate similar large-scale configuration of the magnetic field except for some differences in numerical quantity. As conclusion, the authors point out the necessity and problems of developing a new theory of algorithm for the global coronal magnetic field.
Wang Dong
Wei Fengsi
Yan Yihua
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