Figure 1 from Fundamental Electromagnetic Emissions by a Weak Electron Beam in Solar Wind Plasmas with Density Fluctuations

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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}﹩.

Other Images in This Article

Copyright and Terms & Conditions