Stellar Chromospheric Variability
Cool stars with convective envelopes of spectral types F and later tend to exhibit magnetic activity throughout their atmospheres. The presence of strong and variable magnetic fields is evidenced by photospheric starspots, chromospheric plages and coronal flares, as well as by strong Ca <span style=...
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| Principais autores: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
MDPI AG
2021-11-01
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| Colecção: | Universe |
| Assuntos: | |
| Acesso em linha: | https://www.mdpi.com/2218-1997/7/11/440 |
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