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. 2016 Sep 5;121(9):8228–8236. doi: 10.1002/2016JA022547

Figure 2.

Figure 2

IMAGE HENA and TWINS demonstrated that magnetospheric ion precipitation leads rather to an intense albedo of backscattered ENAs (or LAE), than to an empty upward loss cone. The ENA emissions come from a thin (~10 km) layer at about 300 km altitude [Bazell et al., 2010].