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Kinetic Simulation of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. IV. Electron Heating

  • Authors: Artem Bohdan, Martin Pohl, Jacek Niemiec, Paul J. Morris, Yosuke Matsumoto, Takanobu Amano, and Masahiro Hoshino

2020 The Astrophysical Journal 904 12.

  • Provider: AAS Journals

Caption: Figure 3.

Comparison of the model temperature ratio with Cassini measurements during Saturn’s bow shock crossings with ﹩{M}_{{\rm{A}}}\gt 20﹩ and ﹩{\theta }_{{B}_{n}}\gt 45^\circ ﹩ (Masters et al. 2011). Red solid line represents the heating model (Equation (16)), and red dotted lines are the error bars. Green dots are Cassini measurements, with black arrows pointing to the uncorrected values.

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