The transmission of upstream waves to the magnetosphere: an analysis at widly separated ground stations

Physics

Scientific paper

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[2730] Magnetospheric Physics / Magnetosphere: Inner, [2731] Magnetospheric Physics / Magnetosphere: Outer, [2752] Magnetospheric Physics / Mhd Waves And Instabilities, [2784] Magnetospheric Physics / Solar Wind/Magnetosphere Interactions

Scientific paper

In this work we examine some aspects of the penetration and propagation in the terrestrial magnetosphere of upstream waves observed by Cluster, in front of the bow shock, during a minimum of the solar activity (Whole Heliosphere Interval - Carrington Rotation number 2068). The analysis concerns several intervals during which Cluster is in proximity of the bow-shock and the interplanetary conditions are favorable for the waves onset. The Cluster data are compared with magnetospheric observations and ground measurements, both at low latitude and in Antarctica. Particular attention is dedicated to the aspects of the transit time, propagation paths and energy transfer to different ground stations.

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