Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment
A central problem of space plasma physics is how protons and electrons are heated in a turbulent, magnetized plasma. The differential heating of charged species due to dissipation of turbulent fluctuations plays a key role in solar wind evolution. Measurements from previous heliophysics missions hav...
| المؤلفون الرئيسيون: | , , , , , , , , , , , , , |
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| التنسيق: | مقال |
| اللغة: | English |
| منشور في: |
IOP Publishing
2023-01-01
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| سلاسل: | The Astrophysical Journal Letters |
| الموضوعات: | |
| الوصول للمادة أونلاين: | https://doi.org/10.3847/2041-8213/acf85e |