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Interpretation of the IBEX-Lo Observations of Energetic Neutral Atoms along the Voyager Trajectories

  • Authors: Federico Fraternale, Ratan Bera, Nikolai V. Pogorelov, Eric J. Zirnstein, Vadim Roytershteyn

Federico Fraternale et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 2.

Proton fluxes, ﹩J({E}^{{\prime} })={v}^{2}f(v)/{m}_{p}﹩, are presented as functions of energy, ﹩{E}^{{\prime} }﹩, in the plasma reference frame. Panel (a): hybrid-simulation-derived distributions of thermal protons (blue circles) and PUIs (red circles) downstream of the TS. The fitted double-κ distributions for both populations are shown with the thin lines. Panel (b): example of the evolved VDFs deep in the IHS along the V1 LOS (symbols), compared with the corresponding thermal-proton and PUI VDFs from simulation B obtained using the TS VDF model without loss or injection due to charge exchange (thin blue and red lines, respectively). Panel (c): streamline lengths. Panel (d): the convective times from the TS to the radial point on the LOS.

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