Cross-scale energy cascade powered by magnetospheric convection

Plasma convection in the Earth’s magnetosphere from the distant magnetotail to the inner magnetosphere occurs largely in the form of mesoscale flows, i.e., discrete enhancements in the plasma flow with sharp dipolarizations of magnetic field. Recent spacecraft observations suggest that the dipolariz...

Descripción completa

Detalles Bibliográficos
Autores principales: Ukhorskiy, Aleksandr Y., Sorathia, Kareem A., Merkin, Viacheslav G., Crabtree, Chris, Fletcher, Alex C., Malaspina, David M., Schwartz, Steven J.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8924280/
https://www.ncbi.nlm.nih.gov/pubmed/35292669
http://dx.doi.org/10.1038/s41598-022-08038-x