Study of the formation of Kelvin-Helmholtz instability and shocks in coronal mass ejections

Study of the formation of Kelvin-Helmholtz instability and shocks in coronal mass ejections

The coronal mass ejections (CMEs) are phenomena that evidence the complex solar activity. During the CME evolution in the solar wind (SW) the shock and sheath (Sh) are established. With these, the transfer of energy and shock thermalization have origin through several processes like instabilities an...

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Bibliographic Details
Main Author: Murcia, Miguel Andres Paez
Other Authors: Pereira, Vera Jatenco Silva
Format: Others
Language:en
Published: Biblioteca Digitais de Teses e Dissertações da USP 2018
Subjects:
emissão de partculas
instabilidades
instabilities
ondas de choque
particle emission
shock waves
Sol: campos magnéticos
Sol: ejeções de massa coronal (CMEs)
solar wind
Sun: coronal mass ejections (CMEs)
Sun: magnetic fields
vento solar
Online Access:http://www.teses.usp.br/teses/disponiveis/14/14131/tde-03112018-200210/

Internet

http://www.teses.usp.br/teses/disponiveis/14/14131/tde-03112018-200210/

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