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. 2020 Aug 12;7(8):e2019EA000938. doi: 10.1029/2019EA000938

Figure 5.

ess2539-fig-0005

Estimated local solar times for all analyzed ejection events with error bars indicating 1‐sigma uncertainties. Both near and far solutions are shown for all events except those for which one solution could be ruled out either through independent solutions from Leonard et al. (2020) or through observations of particles in front of Bennu indicating that the far solution was not plausible.