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. 2022 May 9;218(4):28. doi: 10.1007/s11214-022-00895-2

Fig. 13.

Fig. 13

SWAP observations at 25.7 au from the Sun. The spectrum is color-coded to show the primary source of the counts. The blue spectra identify the H+ PUI observations that are fit with a generalized filled-shell distribution. From McComas et al. (2017b). © AAS. Reproduced with permission