Extended Data Fig. 4: MCMC constrained maps of the thermal and suprathermal electron parameters.
From: Solar flare accelerates nearly all electrons in a large coronal volume
a, Thermal electron number density nth. For each pixel, the median value of the MCMC probability distribution is shown. b, Similar to a but for the non-thermal electron number density nnth. c, Map of the ratio of the upper limit of the thermal number density \({n}_{{\rm{th}}}^{{\rm{upper}}}\) (defined as one σ above the median \({n}_{{\rm{th}}}+{\sigma }_{{n}_{{\rm{th}}}}\)) to the non-thermal number density nnth. d, Similar to a but for the low-energy cut-off Emin.
