Fig. 3From: Simulation study on parametric dependence of whistler-mode hiss generation in the plasmasphereSpatial and temporal evolution (\(t=0\sim 4.2\times 10^4[\Omega _{e0}^{-1}]\)) of amplitudes of forward-propagating waves in a Case 1 (\(a=1.87\times 10^{-7}(\Omega _{e0}/c)^2\)); b Case 2 (\(a=3.74\times 10^{-6}(\Omega _{e0}/c)^2\)), and c Case 3 (\(a=3.74\times 10^{-5}(\Omega _{e0}/c)^2\)), respectively. The dashed white lines indicate the magnetic equatorBack to article page