Image Details
Caption: Figure 10.
Downstream energy spectra of electrons: ﹩{\sigma }_{e}=3\times {10}^{-1}﹩ (left) and ﹩{\sigma }_{e}=3\times {10}^{-3}﹩ (right). The black dashed lines in the left and right panels indicate a 2D relativistic Maxwellian and a power-law distribution fitting result, respectively.
© 2017. The American Astronomical Society. All rights reserved.