THE Fe  XXV EXCITATION EQUILIBRIUM IN THE SOLAR CORONA FOR THE ELECTRON POWER DISTRIBUTIONS USING A PSEUDO-TEMPERATURE

@article{Dzifkov2001THEF,
  title={THE Fe  XXV EXCITATION EQUILIBRIUM IN THE SOLAR CORONA FOR THE ELECTRON POWER DISTRIBUTIONS USING A PSEUDO-TEMPERATURE},
  author={Elena Dzif{\vc}{\'a}kov{\'a} and Alena Kulinov{\'a}},
  journal={Solar Physics},
  year={2001},
  volume={203},
  pages={53-70}
}
The excitation equilibrium of Fe xxv in the solar corona for electron power distributions is presented. A parametric form of the distribution function is used to demonstrate the changes in the excitation equilibrium due to the shape of the distribution. A pseudo-temperature is used for better understanding of the changes in the excitation equilibrium. The Fe xxv line intensities depend on the shape of the electron distribution and unusual Fe line ratios can be observed for non-thermal… CONTINUE READING

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