Abstract. We present some methods of X-ray data analysis employed in our laboratory for deducing the physical parameters of flaring plasma. For example, we have used a flare well observed with Polish instrument RESIK aboard Russian CORONAS-F satellite. Based on a careful instrument cali-bration, the absolute fluxes in a number of individual spectral lines have been obtained. The analysis of these lines allows us to follow the evolution of important thermodynamic parameters characterizing the emitting plasma throughout this flare evolution. Key words. Sun—flares—X-rays—spectroscopic plasma diagnostic. 1
This paper describes the methods used to obtain the thermal evolution and radiative output during so...
The temperature reached by solar flares is a key parameter to understanding the physical process tha...
We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) ...
Solar flare is a phenomenon during which a large amount of energy is released in various forms. Part...
This thesis starts with an overview of the physics of the solar corona, concentrating on X-ray emiss...
The aim of the thesis is the study of properties of solar flares via reconstruction of energy distri...
Aims. We aim to prove and diagnose the occurrence of nonthermal electron distributions in solar flar...
The 3.8–10 keV solar flare spectrum includes lines of highly stripped Ca, Fe, and Ni ions, as well a...
Aims. To perform a benchmark analysis for the recent version of the CHIANTI atomic database (v. 5.2)...
The 4-10 keV solar flare spectrum includes highly excited lines of stripped Ca, Fe, and Ni ions as w...
Abstract. Solar X-ray Spectrometer (SOXS), the first space-borne solar astronomy experiment of India...
Solar flares are magnetic reconnection events resulting in sudden bursts of electromagnetic energy, ...
This thesis strives to improve our understanding of solar activity, specifically the behaviour of so...
A spectral atlas of X-ray lines in the wavelength range 7.47-18.97 Angstroms is presented, based on ...
Abstract—RATAN-600 multiwavelength observations of the Sun reveal sharp spectral inhomogeneities in ...
This paper describes the methods used to obtain the thermal evolution and radiative output during so...
The temperature reached by solar flares is a key parameter to understanding the physical process tha...
We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) ...
Solar flare is a phenomenon during which a large amount of energy is released in various forms. Part...
This thesis starts with an overview of the physics of the solar corona, concentrating on X-ray emiss...
The aim of the thesis is the study of properties of solar flares via reconstruction of energy distri...
Aims. We aim to prove and diagnose the occurrence of nonthermal electron distributions in solar flar...
The 3.8–10 keV solar flare spectrum includes lines of highly stripped Ca, Fe, and Ni ions, as well a...
Aims. To perform a benchmark analysis for the recent version of the CHIANTI atomic database (v. 5.2)...
The 4-10 keV solar flare spectrum includes highly excited lines of stripped Ca, Fe, and Ni ions as w...
Abstract. Solar X-ray Spectrometer (SOXS), the first space-borne solar astronomy experiment of India...
Solar flares are magnetic reconnection events resulting in sudden bursts of electromagnetic energy, ...
This thesis strives to improve our understanding of solar activity, specifically the behaviour of so...
A spectral atlas of X-ray lines in the wavelength range 7.47-18.97 Angstroms is presented, based on ...
Abstract—RATAN-600 multiwavelength observations of the Sun reveal sharp spectral inhomogeneities in ...
This paper describes the methods used to obtain the thermal evolution and radiative output during so...
The temperature reached by solar flares is a key parameter to understanding the physical process tha...
We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) ...