Sarah Matthews Submitted: 07-Oct-2002 10:28
Combine RHESSI with complementary datasets, including UV imaging, EUV imaging and spectroscopy and magnetic field
information to determine the conditions that lead to pre-flare activity and its relationship to subsequent energy release. Also to determine the conditions that don't lead to pre-flare activity but still produce a flare.
Participants: Sarah Matthews, Louise Harra, Lucie Green & Len Culhane
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