Figure 5.
Mars’ halo emission spectrum folded through the LEM spectral response, during quiescence (top) and transient (bottom) conditions. Left to right columns show the spectra using the instrumental effective areas as described in the main text: (1) No optical blocking filter, (2) With a thin optical filter, (3) With a thick optical filter.

Mars’ halo emission spectrum folded through the LEM spectral response, during quiescence (top) and transient (bottom) conditions. Left to right columns show the spectra using the instrumental effective areas as described in the main text: (1) No optical blocking filter, (2) With a thin optical filter, (3) With a thick optical filter.

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