The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 so lar radii, encompasses almost all of the influential physical transitions and processes that govern the behavior of coronal outflow ...

Srivastava et al. (2010) have observed a highly twisted coronal loop, which was anchored in AR10960 during the period 04:43 UT- 04:52 UT on 4 June 2007. The loop length and radius are approximately 80 Mm and 4 Mm, with a ...