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Injection Process of Pickup Ion Acceleration at an Oblique Heliospheric Termination Shock

  • Authors: Shuichi Matsukiyo, Yosuke Matsumoto

Shuichi Matsukiyo and Yosuke Matsumoto 2024 The Astrophysical Journal Letters 970 .

  • Provider: AAS Journals

Caption: Figure 2.

Particle distribution and magnetic fields upstream of the shock at t = 65 (Θ Bn = 50°). From the top, V x x phase-space distributions of (a) PUIs, (b) SWIs, (c) electrons; magnetic field components of (d) B x , (e) B y , (f) B z ; and velocity distributions of PUIs at (g) x = 200, (h) x = 300, and (i) x = 400. In panels (a)–(c) and (g)–(i), only the particles at yL y /2 are counted. The color bars in panels (a)–(c) denote phase-space density (in an arbitrary unit). The color bar in panels (g)–(i) denotes velocity space density (in an arbitrary unit). The dashed lines in panels (g)–(i) represent the direction of local (upstream) magnetic field, B 0.

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