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For accurate spectral diagnostics in the solar transition region, we discuss the electron energies for non-Maxwellian distributions both for and Druyvesteyn distributions. We analyze the difference between the κ and… Click to show full abstract
For accurate spectral diagnostics in the solar transition region, we discuss the electron energies for non-Maxwellian distributions both for and Druyvesteyn distributions. We analyze the difference between the κ and the Druyvesteyn distributions with the Maxwellian distribution and derive the expressions for the averaged collision strengths for the κ and the Druyvesteyn distributions. This discussion will be significant for spectral diagnostics of the electron density and temperature in the solar transition region.
Journal Title: Journal of the Korean Physical Society
Year Published: 2017
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