Radial Evolution of Non-Maxwellian Electron Populations Derived from Quasi-thermal Noise Spectroscopy: Parker Solar Probe Observations
Understanding the transport of energy within space plasmas, particularly in the solar wind, remains a complex challenge. Accurate measurement of electron temperatures and their nonthermal characteristics is crucial for comprehending energy transport properties in plasmas. Quasi-thermal-noise (QTN) s...
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          | Main Authors: | , , , , , , , , , , | 
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| Format: | Article | 
| Language: | English | 
| Published: | IOP Publishing
    
        2024-01-01 | 
| Series: | The Astrophysical Journal | 
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad7d05 | 
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