Magnetic structure of an activated filament in a flaring active region

C. Sasso; A. Lagg; S. K. Solanki

doi:10.1051/0004-6361/201322481

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Volume 561 (January 2014)

A&A, 561 (2014) A98

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Fig. 4

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Left: map of the chromospheric magnetic field strength. Right: map of the mean value of the retrieved v_LOS for the He components weighted with the respective filling factor α. Red and black contours outline the position of the filament as sampled by the spectropolarimeter’s scan. They are defined as I^∗ = ^∫(I_c − I)dλ = 2 × 10⁴ counts (see left panel of Fig. 3).

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