Fig. 6

Simulated spin phase-integrated total counts of NIS D per orbit, compared with the total counts of D atoms sputtered off by NIS He atoms from the terrestrial water layer on the IBEX-Lo conversion surface (grey) for the interval in 2010 when the counts from the sputtered component are comparable with the counts from NIS D. See Table 3. Note that these atoms almost solely come from the secondary population.
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