The diagnostic temperature discrepancy as evidence for non-Maxwellian coronal electrons
Victor Edmonds

TL;DR
The paper presents evidence for non-Maxwellian electron velocity distributions in the solar corona, based on persistent temperature diagnostic discrepancies and modeling with kappa distributions.
Contribution
It introduces the idea that non-Maxwellian electron distributions explain the temperature discrepancy, supported by observational data and theoretical modeling.
Findings
Radio diagnostics yield T_e ~ 0.6 MK and T_e ~ 1.5 MK, with a factor of 2.4 discrepancy.
The temperature ratio R is cycle-invariant despite turbulence variations.
Kappa distribution models with kappa ~ 2-3 match the observed ratio R.
Abstract
Two independent electron temperature diagnostics applied to the quiet solar corona yield systematically different results. Radio brightness temperatures from the Nancay Radioheliograph indicate T_e ~ 0.6 MK, while hydrostatic scale-height modeling requires T_e ~ 1.5 MK. Both probe electrons; they disagree by a factor of R = 2.4 +/- 0.3. This discrepancy persists across eight years spanning solar minimum and is confirmed by LOFAR at lower frequencies. We consider turbulent scattering, which suppresses brightness temperature, but comparison with the FORWARD/PSIMAS Maxwellian model shows the standard thermal structure predicts ~1.6 MK; scattering accounts for the reduction toward observed MWA values but not the gap to 620 kK. The ratio R is also cycle-invariant despite measured variations in turbulence. We propose the residual discrepancy reflects non-Maxwellian electron velocity…
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