Abstract
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.
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Arnaud, M. and Rothenflug, R., An Updated Evaluation of Recombination and Ionization Rates, Astron. Astrophys., 1985, vol. 60, pp. 425–457.
Arnaud, M. and Raymond, J.C., Iron Ionization and Recombination Rates and Ionization Equilibrium, Astrophys. J., 1992, vol. 398, pp. 394–406.
Batstone, R.M., Evans, K., Parkinson, J.H., and Pounds, K.A., Further X-Ray Spectra of Solar Active Regions, Sol. Phys., 1970, vol. 13, pp. 389–400.
Dere, K.P., Horan, D.M., and Kreplin, R.W., A Multi-Thermal Analysis of Solar X-Ray Emission, Sol. Phys., 1974, vol. 36, pp. 459–472.
Dere, K.P., Landi, E., Mason, H.E., et al., CHIANTI—An Atomic Database for Emission Lines, Astron. Astrophys., 1997, vol. 125, pp. 149–173.
Kepa, A., Sylwester, J., Sylwester, B., and Siarkowski, M., First Determinations of Differential Emission Measure Distribution from RESIK X-Ray Spectra, Proc. IAU Symp. No. 233, 2004, pp. 461–462.
Mazzotta, P., Mazzitelli, G., Colafrancesco, S., and Vittorio, N., Ionization Balance for Optically Thin Plasmas: Rate Coefficients for All Atoms and Ions of the Elements H to NI, Astron. Astrophys., 1998, vol. 133, pp. 403–409.
Pottasch, S.R., On the Interpretation of the Solar Ultraviolet Emission Line Spectrum, Space Sci. Rev., 1964, vol. 3, pp. 816–855.
Shull, J.M. and van Steenberg, M., The Ionization Equilibrium of Astrophysically Abundant Elements, Astrophys. J., Suppl., 1982, vol. 48, pp. 95–107.
Sylwester, J., Schrijver, J., and Mewe, R., Multitemperature Analysis of Solar X-Ray Line, Emission, Sol. Phys., 1980, vol. 67, pp. 285–309.
Sylwester, J., Gaicki, I., Kordylewski, Z., et al., RESIK: A Bent Crystal X-Ray Spectrometer for Studies of Solar Coronal Plasma Composition, Sol. Phys., 2005, vol. 226, pp. 45–72.
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Original Russian Text © A. Kepa, J. Sylwester, B. Sylwester, M. Siarkowski, A.I. Stepanov, 2006, published in Astronomicheskii Vestnik, 2006, Vol. 40, No. 4, pp. 323–330.
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Kepa, A., Sylwester, J., Sylwester, B. et al. Determination of differential emission measure from X-ray solar spectra registered by RESIK aboard CORONAS-F . Sol Syst Res 40, 294–301 (2006). https://doi.org/10.1134/S0038094606040058
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DOI: https://doi.org/10.1134/S0038094606040058