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Fig. 9

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Relative densities (scaled to the values at TS, Eq. (32)) for NIS He, Ne, and O for the four IBEX sampling seasons, calculated for the apogee times of IBEX orbits for the inflow parameters obtained by Bzowski et al. (2012) from IBEX NIS He observations. The vertical bars mark the longitudes of IBEX apogees in 2009, the horizontal bars marks the relative density levels for this time and location in space.

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