“…There is a slight fall in T. during the afterglow period of spontaneous emission, shown in the upper curve of figure 5, which is about half the size of the fall in T, calculated from measurements of the electron density (Loveland and Webb 1992). Although T, and T. are not necessarily related, it is worth noting that the greater fall, in x, is for higher buffer gas pressure of 330mbar, compared with loombar, which results in a greater cooling rate of the electrons.…”