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Solar Coronal Jets: Observations, Theory, and Modeling
Chromospheric and coronal jets represent important manifestations of ubiquitous solar transients, which may be the source of significant mass and energy input to the upper solar atmosphere and the solar wind. While the energy involved in a jet-like event is smaller than that of “nominal” solar flare...
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| Publié dans: | Space Sci Rev |
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| Auteurs principaux: | , , , , , , , , , , , , , , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
2016
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| Sujets: | |
| Accès en ligne: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7477949/ https://ncbi.nlm.nih.gov/pubmed/32908324 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1007/s11214-016-0260-5 |
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