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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 2.

1D profiles of the total fluctuation energy, ﹩{E}_{T}=\lt \delta {v}_{e}^{2}\gt +\lt \delta {b}^{2}/4\pi \rho \gt ﹩, defined by the electron velocity fluctuations δve and ρ = mine, averaged over the Y-​axis at ΩciT = 500. The total energy is normalized by ﹩{v}_{A}^{2}﹩.

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