Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause
Our purpose is to characterize the evolution of the magnetopause Kelvin-Helmholtz (KH) wave activity with changes in thickness of the adjacent boundary layer, geomagnetic latitude and interplanetary magnetic field (IMF) orientation. As the IMF turns northward, wave activity may be generated at the d...
Guardado en:
Autores principales: | Foullon, C., Farrugia, C.J., Fazakerley, A.N., Owen, C.J., Gratton, F.T., Torbert, R.B. |
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Formato: | JOUR |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_21699402_v113_n11_p_Foullon |
Aporte de: |
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