So AR 11520 has not returned after its second transit of the solar far-side. This 'rough' sketch of coronal loops above the AR11520 site on July 18 (as it passes behind the limb) is posted to show some of the southern giant's more extreme behaviour. I will eventually redraw it for presentation. The physics of the loops formation is discussed in earlier posts - they are one of the most beautiful sights anywhere - and notoriously hard to photograph. Webcam users have the best chance as the bright loops saturate in most photos. The human eye almost never saturates, and can see the thin brilliant loops - and follow the tiny bright droplets of condensate (~3000km dia) as they slide down the loops to the flare ribbon sites. The ribbons were no longer visible to me, the M1.7 flare was eight hours earlier. These loops were growing faint - but superb nonetheless. The tall straight ones may be edge-on loops or surges caught up in the event.
The grid lines are 20,000Km apart and the loops are a little above 100,000km (100Mm) high.