A high resolution (~0.5A) spectrum covering the yellow part of the spectrum including the sodium D doublet wavelengths.

The Sodium emission dominates the spectrum. (There is as much light from the two narrow sodium lines as in the rest of the light in this spectrum combined.) There are no other strong emission lines in this yellow part of the spectrum (the Swan bands are further to the blue-green) but there are some other faint emission lines though which I have not yet been able to identify.

We can measure Doppler shifts to calculate the comet's motion both relative to us and to the Sun using the sodium light pollution and daylight spectrum as references

The Doppler shift in the sodium emission lines gives the velocity relative to Earth directly = -55 km/s (ie the comet is moving towards us)

We see the Sun's absorption line spectrum in the sunlight scattered from the comet dust. These absorption lines experience two Doppler shifts, first due to the motion relative to the Sun and then after scattering due to the motion relative to Earth. This total shift = -23km/s

The motion of the comet relative to the Sun is therefore -23 +55 = +32 km/s (ie the comet is moving away from the Sun) These are in good agreement with the values given on the  JPL Horizons website ( -54.9km/s and +31.4 km/s for the time of the observation)