Spatiotemporal Low First Ionization Potential Abundance: A Catalyst for Coronal Condensation
Radiative losses play a critical role in the cooling of plasmas. When chromospheric plasma is sufficiently heated, it can flow into coronal loops, which subsequently cool down due to radiation. From observations, we infer that this cooling does not occur uniformly, often resulting in coronal condens...
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| Principais autores: | , , , |
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| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
IOP Publishing
2025-01-01
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| Serija: | The Astrophysical Journal |
| Teme: | |
| Online dostop: | https://doi.org/10.3847/1538-4357/ae019d |
| Oznake: |
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