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 instabilitie...

Full description

Bibliographic Details
Main Author: Miguel Andres Paez Murcia
Other Authors: Vera Jatenco Silva Pereira
Language:English
Published: Universidade de São Paulo 2018
Subjects:
emissão de partculas
instabilidades
ondas de choque
Sol: campos magnéticos
Sol: ejeções de massa coronal (CMEs)
vento solar
instabilities
particle emission
shock waves
solar wind
Sun: coronal mass ejections (CMEs)
Sun: magnetic fields
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/

Similar Items