Hugh Hudson Submitted: 28-Mar-2003 08:51
The RHESSI low-energy spectra show the Fe complex at 6-7 keV as
an extremely prominent feature that can be characterized quite precisely within the resolution of the instrument. In principle this feature and
the neighboring continuum give several pieces of information about
the tail of the thermal plasma in a flare. We are hoping to see non-equilibrium effects, or other interesting properties, by looking at fast flares for which the shutters remained in place.
Participants: B.R. Dennis, H.S. Hudson, K.J.H. Phillips, R.A. Schwartz, and D.M. Smith
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