Fig. 1From: Simulation study on parametric dependence of whistler-mode hiss generation in the plasmaspherea Initial velocity distribution of hot electrons with the parabolic gradient coefficient of the background magnetic field \(a=1.87\times 10^{-7}(\Omega _{e0}/c)^2\) (i.e., Case 1) in the space range of \(h=-50 \sim 50[c\Omega _{e0}^{-1}]\); b variation of the velocity distribution at \(t=20480[\Omega _{e0}^{-1}]\)Back to article page