Physics
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sosyr..40..294k&link_type=abstract
Solar System Research, Volume 40, Issue 4, pp.294-301
Physics
3
96.60.Ub
Scientific paper
The differential emission measure (DEM) describes the temperature distribution of the emitting plasma. The DEM distribution allows one to study the physical conditions and the energy of flares in detail (including the mean temperature and the total emission measure). In this paper, we analyze the time changes of the DEM distributions for a selected flare, which has been observed with the RESIK instrument. To calculate the differential emission measure, we used the Withbroe-Sylwester (W-S) iterative algorithm corresponding to the maximum likelihood procedure. The required emission functions were calculated with the CHIANTI package. We calculated the DEM for four available estimates of the ionization equilibrium and coronal composition of plasma.
Kepa Anna
Siarkowski Marek
Stepanov I. A.
Sylwester Barbara
Sylwester Janusz
No associations
LandOfFree
Determination of differential emission measure from X-ray solar spectra registered by RESIK aboard CORONAS-F does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Determination of differential emission measure from X-ray solar spectra registered by RESIK aboard CORONAS-F, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of differential emission measure from X-ray solar spectra registered by RESIK aboard CORONAS-F will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1618691