Authors: L.
Fletcher & H. Hudson.
·
Figure 2
Pairwise correlation plots of broad-band flux ratios for the four
flares studied, with the harder and softer bands set with
boundaries at 10, 20, 30, 50 and 70 keV. The 'hysteresis'
loops at the lowest energies (black crosses) show the presence of
an uncorrelated slowly-varying component, identified with
the hot flare plasma or the 'super-hot' component reported
by Lin and Schwartz (1987). Yellow stars show the ratio of 30-20
to 50-30 keV fluxes. At the highest energies (blue
diamonds) the correlation is almost the same for burst
rise and fall.
·
Figure 3
Footpoint locations for each of the four flares derived from the CLEAN
maps. These are colour-coded by time.
· Figure 5 :
CLEAN source centroids (as opposed to CLEAN map centroids) during the
14 March 2002 flare, showing systematic motion along a ribbon.
·
Postscript Versions of all Figures