This week's nugget continues to waffle on with a theme evolving from several previous nuggets regarding transequatorial N-S coronal loops. The new remarkable feature of this week's phenomena is the involvement of the NS loop connections with newly emerging flux and with active-region expansions. To summarize the problems these loops present us with...
But how does the reconnection proceed, what drives it, and what are its consequences? We note from previous nuggets that the NS loops show up quite well in Yohkoh/SXT images, which immediately implies high temperature and suggests a signature for the reconnection. S. Tsuneta suggested that loops rising from active regions could drive the reconnection. Do this week's remarkable observations fit this idea?
An MDI and an SXT image from that epoch:
A registered (thanks, Dom) image pair at higher resolution
A short movie:
A longer movie:
Really, there is a lot of speculation that can result from these beautiful data. We hasten to note that the SXT images are from our first-pass data reduction, and we will later have more data with higher quality. But we think we see the following features, mainly found from the long movie:
It is a bit baffling. We seem to have caught large-scale magnetic reconnection in the act, and yet we don't see dramatic consequences. Nevertheless, the loops are hot (measurements to be made, but "hot" by comparison with SOHO EUV standards) and require energy input, but it does not seem to be happening suddenly. Perhaps the most logical inference would be that the reconnection is proceeding in a gradual and benign manner, and that the NS loops largely have been in place prior to the active-region flux emergences (a "super-canopy"?).
July 9, 1999: Brian Handy, Hugh Hudson