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...

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Detalles Bibliográficos
Publicado:	2008
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_21699402_v113_n11_p_Foullon http://hdl.handle.net/20.500.12110/paper_21699402_v113_n11_p_Foullon
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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