Add to ORKGThe effects of the reduction in the thermal conductivity due to heavy ions on electron temperatures in the solar corona and solar wind are examined. Large enhancements of heavy ions in the corona appear to be necessary to give appreciable changes in the thermal gradient of the electrons
We examine the effects of including effects of both protons and electrons on the heating of the fast...
Solar wind heavy ion spectra measured with the Vela instrumentation have been studied with the goal ...
The dynamic behavior of the plasma in the chromosphere/transition region /inner corona is vital for ...
The electron temperature profile in the polar coronal hole inferred by the ionic charge state data o...
A comparison of polar solar wind proton flux upper limits derived using a coronal density model, wit...
The temperatures of some highly charged ions in the southern solar polar coronal hole are determined...
The presence of suprathermal electrons has important consequences on the acceleration process of the...
Diffusion of heavy ions in solar corona studied with one-fluid and two-fluid dynamic model
In the solar corona the collisional mean free path λ for a thermal particle (electrons or protons) i...
Heavy ions in the solar wind are ideal for studying injection processes in the solar wind. We use co...
The development of knowledge of how the coronal origin of the solar wind affects its in situ propert...
Coronal expansion effect on calculation of electron temperature from emission-line intensitie
Physical quantities, such as ion temperature and nonthermal velocity, provide critical information a...
A simple model of the lower corona which allows for a possible difference in the electron and proton...
The goal of the proposed research was to increase the understanding of coronal plasma phenomena by m...
We examine the effects of including effects of both protons and electrons on the heating of the fast...
Solar wind heavy ion spectra measured with the Vela instrumentation have been studied with the goal ...
The dynamic behavior of the plasma in the chromosphere/transition region /inner corona is vital for ...
The electron temperature profile in the polar coronal hole inferred by the ionic charge state data o...
A comparison of polar solar wind proton flux upper limits derived using a coronal density model, wit...
The temperatures of some highly charged ions in the southern solar polar coronal hole are determined...
The presence of suprathermal electrons has important consequences on the acceleration process of the...
Diffusion of heavy ions in solar corona studied with one-fluid and two-fluid dynamic model
In the solar corona the collisional mean free path λ for a thermal particle (electrons or protons) i...
Heavy ions in the solar wind are ideal for studying injection processes in the solar wind. We use co...
The development of knowledge of how the coronal origin of the solar wind affects its in situ propert...
Coronal expansion effect on calculation of electron temperature from emission-line intensitie
Physical quantities, such as ion temperature and nonthermal velocity, provide critical information a...
A simple model of the lower corona which allows for a possible difference in the electron and proton...
The goal of the proposed research was to increase the understanding of coronal plasma phenomena by m...
We examine the effects of including effects of both protons and electrons on the heating of the fast...
Solar wind heavy ion spectra measured with the Vela instrumentation have been studied with the goal ...
The dynamic behavior of the plasma in the chromosphere/transition region /inner corona is vital for ...