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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Détails bibliographiques
Publié dans:Space Sci Rev
Auteurs principaux: Raouafi, N. E., Patsourakos, S., Pariat, E., Young, P. R., Sterling, A., Savcheva, A., Shimojo, M., Moreno-Insertis, F., DeVore, C. R., Archontis, V., Török, T., Mason, H., Curdt, W., Meyer, K., Dalmasse, K., Matsui, Y.
Format: Artigo
Langue:Inglês
Publié: 2016
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Article
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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