Second Harmonic Electromagnetic Wave Emissions from a Turbulent Plasma with Random Density Fluctuations
In the solar wind, electromagnetic waves at the harmonic plasma frequency 2 ω _p can be generated as a result of coalescence between forward- and backward-propagating Langmuir waves. A new approach to calculate their radiation efficiency in plasmas with external background density fluctuations is de...
| Hlavní autoři: | , |
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| Médium: | Článek |
| Jazyk: | English |
| Vydáno: |
IOP Publishing
2024-01-01
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| Edice: | The Astrophysical Journal |
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| On-line přístup: | https://doi.org/10.3847/1538-4357/ad20ee |