Hugh Hudson Submitted: 06-Feb-2008 09:18
The high-resolution data from Hinode make a renewed search for preflare
structures interesting. With Yohkoh resolution, it was found that flare
loops were normally not visible in soft X-rays prior to the event. We
propose to carry out a new search of this type, taking advantage of RHESSI and SOT data for footpoint location, XRT for loop structure, and EIS data for
preflare loop temperature/density estimations. The main reason for this
study is that the preflare state may provide physical clues to causation.
Participants: H. Hudson, C. Chifor, E. DeLuca I. Hannah, K. Watanabe
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