The Diagnostic Temperature Discrepancy as Evidence for Non-Maxwellian Coronal Electrons
Two independent electron temperature diagnostics applied to the quiet solar corona yield systematically different results. Radio brightness temperatures from the Nançay Radioheliograph indicate Tₑ ≈ 0.6 MK, while hydrostatic scale-height modeling of the same plasma requires Tₑ ≈ 1.5 MK (Mercier & Ch...
Kaydedildi:
| Yazar: | |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
Maynooth Academic Publishing
2026-04-01
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| Seri Bilgileri: | The Open Journal of Astrophysics |
| Online Erişim: | https://doi.org/10.33232/001c.161223 |
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