James McTiernan Submitted: 09-Jan-2004 11:44
This is an ongoing effort to measure T and EM of the Sun
during quiet times, i.e., when no discernable variation in
the RHESSI 3-12 keV count rate can be seen for times > 1
minute. As of 1-jan-2004, we have 3021 good time intervals.
The idea is to compare the high T emission measure with
expectations from heating models, in particular the nanoflare model of Klimchuk and Cargill. To compare with
the model DEM's, we will generate the full-sun DEM using EIT, SXI and RHESSI data.
Participants: J McTiernan J Klimchuk
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