Magnetic Reconnection Inside a Flux Rope Induced by Kelvin‐Helmholtz Vortices

On 5 May 2017, MMS observed a crater‐type flux rope on the dawnside tailward magnetopause with fluctuations. The boundary‐normal analysis shows that the fluctuations can be attributed to nonlinear Kelvin‐Helmholtz (KH) waves. Reconnection signatures such as flow reversals and Joule dissipation were...

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Detalles Bibliográficos
Autores principales: Hwang, K.‐J., Dokgo, K., Choi, E., Burch, J. L., Sibeck, D. G., Giles, B. L., Hasegawa, H., Fu, H. S., Liu, Y., Wang, Z., Nakamura, T. K. M., Ma, X., Fear, R. C., Khotyaintsev, Y., Graham, D. B., Shi, Q. Q., Escoubet, C. P., Gershman, D. J., Paterson, W. R., Pollock, C. J., Ergun, R. E., Torbert, R. B., Dorelli, J. C., Avanov, L., Russell, C. T., Strangeway, R. J.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2020
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7375157/
https://www.ncbi.nlm.nih.gov/pubmed/32714734
http://dx.doi.org/10.1029/2019JA027665

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7375157/
https://www.ncbi.nlm.nih.gov/pubmed/32714734
http://dx.doi.org/10.1029/2019JA027665

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