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Momentum transfer at the high-latitude magnetopause and boundary layers

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Fig. 1. Interplanetary conditions as observed by Wind on 3 De- De-cember 1997. The UT reflects the estimated 70-min lag from Wind to the magnetopause
Fig. 3. Data from the Polar spacecraft pass through the region of cusp aurora. Top to bottom: invariant latitude; ion and electron energy spectrograms; integrated energy and number fluxes for electrons (red) and ions (blue).
Fig. 4. Expanded view of Polar magnetic field and plasma moments from the interval marked I in Fig
Fig. 6. Solar wind from SOHO/CELIAS and IMF from ACE on 21 January 2001. The time refers to the ACE spacecraft and does not include a delay of 75 min (confirmed by observations as discussed in the text)
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