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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...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Argitaratua izan da:Space Sci Rev
Egile Nagusiak: 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.
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: 2016
Gaiak:
Sarrera elektronikoa: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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