  The extremely faint, temperature sensitive ``auroral'' emission line [N II]
5755 has been detected from the low density ionized gas along the sight line
toward l = 130.0, b = -7.5 using the Wisconsin H-Alpha Mapper (WHAM). The
intensity of this emission line, relative to the red nebular line [N II] 6584,
is found to be twice that observed in bright, classical H II regions
surrounding O stars. This implies that the electron temperature of the ionized
gas along this sight line is about 2000 K higher than the H II regions, and
that the enhanced [N II] 6584/H-Alpha and [S II] 6716/H-Alpha intensity ratios
in this low density gas are due at least in part to an elevated temperature.
