Overview of the filament eruption and accompanying flare. Panel (a): SDO/HMI magnetogram. Panel (b): GOES X-ray observations. Panels (c)–(h): SDO/AIA images in 304 Å (c–e) and 131 Å passbands (f–h). The filament and flare loops are indicated. The contour in panel (a) corresponds to 50 DN s⁻¹ px⁻¹ in 304 Å (panel c), showing the relative location of the erupting filament with respect to the photospheric polarities. Dashed and dotted lines indicate the times and the fields of view of Figs. 10, 11, 12. An animation of the SDO/AIA data is available online, spanning 12:50–13:55 UT.