The ULF wave foreshock boundary: Cluster observations

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The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow shock gives rise to a number of plasma instabilities from which ultralow frequency (ULF) waves can grow. Because of their finite growth rate, the ULF waves are spatially localized in the foreshock re...

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Detalles Bibliográficos
Autores principales: Andrés, N., Meziane, K., Mazelle, C., Bertucci, C., Gómez, D.
Formato: INPR
Materias:
Cluster spacecraft
Earth's foreshock
Interplanetary magnetic field
Particle acceleration
Solar wind
ULF waves
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_21699380_v_n_p_Andres
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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