Cargando…
Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions
Solar flares and coronal mass ejections, the primary space weather disturbances affecting the entire heliosphere and near-Earth environment, mainly emanate from sunspot regions harbouring high degrees of magnetic twist. However, it is not clear how magnetic helicity, the quantity for measuring the m...
Autores principales: | Toriumi, Shin, Hotta, Hideyuki, Kusano, Kanya |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2023
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10238451/ https://www.ncbi.nlm.nih.gov/pubmed/37268755 http://dx.doi.org/10.1038/s41598-023-36188-z |
Ejemplares similares
-
Formation and dynamics of a solar eruptive flux tube
por: Inoue, Satoshi, et al.
Publicado: (2018) -
Supergravitational turbulent thermal convection
por: Jiang, Hechuan, et al.
Publicado: (2020) -
Weak influence of near-surface layer on solar deep convection zone revealed by comprehensive simulation from base to surface
por: Hotta, H., et al.
Publicado: (2019) -
Turbulent superstructures in Rayleigh-Bénard convection
por: Pandey, Ambrish, et al.
Publicado: (2018) -
Magnetic Helicity and the Solar Dynamo
por: Shebalin, John V.
Publicado: (2019)