Boundary of the Distribution of Solar Wind Proton Beta versus Temperature Anisotropy
The frequency distribution of solar wind protons, measured in the vicinity of Earth’s orbit, is customarily plotted in ( β _∥ , T _⊥ / T _∥ ) phase space. Here, T _⊥ / T _∥ is the ratio of perpendicular and parallel temperatures, and β _∥ = 8 π nT _∥ / B ^2 is the ratio of parallel thermal energy to...
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| Hlavní autoři: | , , , , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
IOP Publishing
2024-01-01
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| Edice: | The Astrophysical Journal |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/1538-4357/ad47f1 |
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