Add to ORKGThe cross section requirements are presented for studying UV and X-ray emission spectra associated with active and flare-produced plasmas in the sun's corona. The general approach to the calculation of the distorted wave approximation problem is also given
X-ray and ultraviolet line emission from hot, optically thin material forming coronal active regions...
The determination of electron density in the solar atmosphere using diagnostic line ratios has been ...
There is increasing emphasis during this decade on understanding energy balance and phenomena observ...
We have re-analyzed Solar Ultraviolet Measurement of Emitted Radiation (SUMER) observations of a par...
Extending previous studies of nonthermal electron transport in solar flares, which include the effec...
We have re-analyzed Solar Ultraviolet Measurement of Emitted Radiation (SUMER) observations of a par...
Electron collisional excitation rates and transition probabilities are important for computing elect...
X-ray observations are a direct diagnostic of fast electrons produced in solar flares, energized dur...
X-ray observations are a direct diagnostic of fast electrons produced in solar flares, energized dur...
Firstly, we present reviews of the background atomic, magnetohydrodynamic, and solar, physics involv...
Coronal structures receive radiation not only from the solar disc, but also from the corona. This he...
Abstract. Role of many-body interactions on the energy loss of electrons accelerated at neutral poin...
Emission lines from highly-excited states (n ≥ 5) of H- and He-like ions have been detected in astro...
In this paper, we propose that the accelerated electrons in the quiet Sun could collide with the sol...
The study of charge changing cross sections of fast ions colliding with matter provides the fundamen...
X-ray and ultraviolet line emission from hot, optically thin material forming coronal active regions...
The determination of electron density in the solar atmosphere using diagnostic line ratios has been ...
There is increasing emphasis during this decade on understanding energy balance and phenomena observ...
We have re-analyzed Solar Ultraviolet Measurement of Emitted Radiation (SUMER) observations of a par...
Extending previous studies of nonthermal electron transport in solar flares, which include the effec...
We have re-analyzed Solar Ultraviolet Measurement of Emitted Radiation (SUMER) observations of a par...
Electron collisional excitation rates and transition probabilities are important for computing elect...
X-ray observations are a direct diagnostic of fast electrons produced in solar flares, energized dur...
X-ray observations are a direct diagnostic of fast electrons produced in solar flares, energized dur...
Firstly, we present reviews of the background atomic, magnetohydrodynamic, and solar, physics involv...
Coronal structures receive radiation not only from the solar disc, but also from the corona. This he...
Abstract. Role of many-body interactions on the energy loss of electrons accelerated at neutral poin...
Emission lines from highly-excited states (n ≥ 5) of H- and He-like ions have been detected in astro...
In this paper, we propose that the accelerated electrons in the quiet Sun could collide with the sol...
The study of charge changing cross sections of fast ions colliding with matter provides the fundamen...
X-ray and ultraviolet line emission from hot, optically thin material forming coronal active regions...
The determination of electron density in the solar atmosphere using diagnostic line ratios has been ...
There is increasing emphasis during this decade on understanding energy balance and phenomena observ...