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Acceleration of Electrons and Ions by an “Almost” Astrophysical Shock in the Heliosphere

  • Authors: Immanuel Christopher Jebaraj, Oleksiy Agapitov, Vladimir Krasnoselskikh, Laura Vuorinen, Michael Gedalin, Kyung-Eun Choi, Erika Palmerio, Nicolas Wijsen, Nina Dresing, Christina Cohen, Athanasios Kouloumvakos, Michael Balikhin, Rami Vainio, Emilia Kilpua, Alexandr Afanasiev, Jaye Verniero, John Grant Mitchell, Domenico Trotta, Matthew Hill, Nour Raouafi, Stuart D. Bale

Immanuel Christopher Jebaraj et al 2024 The Astrophysical Journal Letters 968 .

  • Provider: AAS Journals

Caption: Figure 4.

Transition region of the quasi-parallel shock. Panel (A) displays the time evolution (depicted by the colors blue to red) of the transversal magnetic field components. The dotted line through the middle represents the mean field, B 0. Panel (B) illustrates a 2D schematic of the shock transition in the plasma frame. The spatial scales are in λ i (represented with 50λ i × 50λ i squares) and are estimated for the upstream and downstream separated at the edge of the quasi-parallel shock (Q ). The gray scale represents the change in B across the shock. The direction of B and the shock normal are also marked by arrows. The dark stripes in the middle represent the quasi-perpendicular structure at the ramp and the whistler precursors. Panel (C) presents the magnetic field magnitude upon which the schematic is based.

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