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Comment: Published by Scroll Versions from space DraftSPEARFIMS and version 1.0

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L-band aurora with dense pattern of vertical emission lines.Image ModifiedS-band aurora with sparse pattern of vertical emission lines.Image ModifiedL-band sky-survey with faint pattern of vertical emission lines.Image ModifiedS-band sky-survey with sparse pattern of vertical emission lines.Image Modified

Figures 1 - (a) corrected L-band aurora, (b) corrected S-band aurora, (c) corrected L-band sky survey, (d) corrected L-band aurora.

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Wavelength fit residuals range from -0.2 to 0.5 Angstroms.Image Modified

Figure 2 - Plots of residuals from second-order polynomial fits to the dispersion solutions for L-band (upper) and S-band (lower) as a function of wavelength.

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