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PUI Acceleration at an Oblique Heliospheric Termination Shock: 2D Hybrid Kinetic Simulation

  • Authors: Masaru Nakanotani, Gary P. Zank, Marc Kornbleuth, Merav Opher

Masaru Nakanotani et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

vx − vy phase space of PUIs upstream of the shock wave in the simulation frame at ΩciT = 50. The core and reflected PUI components are located at around (vx, vy) = (10, 0)vA and ( −15, 33)vA, respectively. The white dashed line corresponds to the direction of the background magnetic field.

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