We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) using SMM X-ray data from Bent Crystal Spectrometer (BCS) and Hard X-ray Imaging Spectrometer (HXIS). We have found that the analysis provide a very sensitive test of consistency of observational data coming from different instruments or different channels of the same instrument. This has allowed to eliminate some systematic differences contained in the analysed data. Typical examples of the DEM distribution are discussed. It is stressed that these improvements in the multitemperature flare diagnostics are very important for the discussion of flare energetics
The Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) has been providi...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
Context. The non-Maxwellian κ-distributions have been detected in the solar wind and can explain int...
We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) ...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
To solve a number of problems in solar physics related to mechanisms of energy release in solar coro...
29 pages, 7 figuresWe analyse the temporal evolution of the Differential Emission Measure (DEM) of s...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The aim of the thesis is the study of properties of solar flares via reconstruction of energy distri...
We perform Differential Emission Measure (DEM) analysis of an M7.7 flare that occurred on 2012 July ...
The temperature distribution of the emitting plasma is a crucial constraint when studying the heatin...
In a previous paper we have described a technique to derive constraints on the differential emission...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) has been providi...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
Context. The non-Maxwellian κ-distributions have been detected in the solar wind and can explain int...
We have investigated differential emission measure (DEM) distribution of hot flare plasma (T>10 MK) ...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
To solve a number of problems in solar physics related to mechanisms of energy release in solar coro...
29 pages, 7 figuresWe analyse the temporal evolution of the Differential Emission Measure (DEM) of s...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The aim of the thesis is the study of properties of solar flares via reconstruction of energy distri...
We perform Differential Emission Measure (DEM) analysis of an M7.7 flare that occurred on 2012 July ...
The temperature distribution of the emitting plasma is a crucial constraint when studying the heatin...
In a previous paper we have described a technique to derive constraints on the differential emission...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
The Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) has been providi...
The detailed knowledge of plasma heating and acceleration region properties presents a major observa...
Context. The non-Maxwellian κ-distributions have been detected in the solar wind and can explain int...