Titile :	Flaring Structures Observed on Deconvolved SXT Images }

Authors:	B. Sylwester and  J.Sylwester

Abstract
We present and discuss evolution of flaring structures morphology as 
observed on deconvolved soft X-ray images. The X-ray images have been 
obtained using the Soft X-ray Telescope (SXT) on {\em Yohkoh}. The 
deconvolution has been made using the iterative maximum likelihood 
algorithm {\em ANDRIL.} On the reconstructed images it is possible to 
study the position of individual fine structures for the first time with 
the resolution superior to the SXT pixel size. We show example of the 
analysis of deconvolved images for one disc flare on 11~July~1992 at 
15:25 UT. These flares are on 19~November~1991 and on 13~January~1992 
and have been located near/at the limb. We conclude about the 
differences of physical conditions of the flaring plasma confined in 
compact bright regions (kernels) located in the footpoint and summit 
areas.



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