Fig. 12.

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Evolution of the atmosphere along a single field line with one footpoint at x = −10 Mm, discussed in Sect. 3.4.1 (B0 = 65 G, x = −10 Mm, F0 = 1.0F10). They are shown in plots of time on the horizontal axis and length, s, along the field line vertically, with s = 0 at x = −10 Mm, y = 0 Mm. The parameters shown are (a) plasma number density, (b) the vertical velocity, (c) the plasma temperature, (d) the kinetic energy density. The plasma number density panel show the beam electron energy flux deposited in the chromosphere above the left footpoint, over-plotted in red. This over-plot is scaled such that the maximum electron energy flux deposited throughout the entire simulation (4.7 × 1010 erg cm−2 s−1) corresponds to the peak reaching top of the panel, with zero at the bottom. The beam in this field line reaches a peak flux of 1.0 × 1010 erg cm−2 s−1. We note that the field line changes in overall length as a function of time. The extent of the experimental domain is highlighted with green lines in each panel. Before reconnection this highlights the bottom and top of the experiment, after reconnection these highlight the locations of the photospheric footpoints in each time step. Values outside of this are saturated to their photospheric values for continuity, but do not represent simulated values.
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