Fig. 2.
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Observations of the filament and the NLFFF reconstruction of the MFR. (a) SDO/AIA 304 Å image at 15:12 UT. (b) Hα image from Cerro Tololo Inter-American Observatory at 15:10 UT. (c) Sampled field lines (in different colors) from the reconstructed magnetic field at 13:24 UT. (d) Segments of magnetic field lines that extend from magnetic dips to a scale height of 300 km (cyan lines) at 13:24 UT.
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