High-frequency heating of the solar wind triggered by low-frequency turbulence
The fast solar wind's high speeds and nonthermal features require that significant heating occurs well above the Sun's surface. Two leading theories seem incompatible: low-frequency "Alfvénic" turbulence, which transports energy outwards and is observed ubiquitously by spacecraft...
| Hlavní autoři: | , , , , , |
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| Médium: | Working paper |
| Jazyk: | English |
| Vydáno: |
arXiv
2021
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