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Fig. 5 | Earth, Planets and Space

Fig. 5

From: Simulation study on parametric dependence of whistler-mode hiss generation in the plasmasphere

Fig. 5

Dynamic spectra of forward-propagating waves (\(t=0\sim 4.2\times 10^4[\Omega _{e0}^{-1}]\)) at locations of \(-100, -50, 0, 50, 100 [c\Omega _{e0}^{-1}]\), gradient coefficient a in three cases are a \(1.87\times 10^{-7}(\Omega _{e0}/c)^2\); b \(3.74\times 10^{-6}(\Omega _{e0}/c)^2\), and c \(3.74\times 10^{-5}(\Omega _{e0}/c)^2\), respectively. Typical wave structures with amplitudes over \(10^{-4.5} [B_0]\) are outlined

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