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Fundamental Electromagnetic Emissions by a Weak Electron Beam in Solar Wind Plasmas with Density Fluctuations

  • Authors: C. Krafft, and P. Savoini

2022 The Astrophysical Journal Letters 924 L24.

  • Provider: AAS Journals

Caption: Figure 1.

Initial distribution of the background plasma density fluctuations δn/n0 in the plane (x, y), corresponding to the average level ﹩{\rm{\Delta }}N=\langle {(\delta n/{n}_{0})}^{2}{\rangle }^{1/2}\simeq 0.05﹩. The size of the box is ﹩{L}_{x}\times {L}_{y}=5792\times 2896{\lambda }_{D}^{2}﹩.

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