The Dipolar Solar Minimum Corona
The large-scale configuration of the UV solar corona at the minimum activity between solar cycles 22 and 23 is explored in this paper. Exploiting a large sample of spectroscopic observations acquired by the Ultraviolet Coronagraph Spectrometer aboard the Solar and Heliospheric Observatory in the two...
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| Format: | Article |
| Language: | English |
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MDPI AG
2021-12-01
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| Series: | Universe |
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| Online Access: | https://www.mdpi.com/2218-1997/7/12/507 |