A Scenario for Origin of Global 4 mHz Oscillations in Solar Corona
We establish a spherically symmetric model of solar atmosphere, which consists of the whole chromosphere and low corona below the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>1.25</mn>&l...
| Main Authors: | , , |
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| Format: | Article |
| Jezik: | English |
| Izdano: |
MDPI AG
2025-01-01
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| Serija: | Universe |
| Teme: | |
| Online dostop: | https://www.mdpi.com/2218-1997/11/1/14 |