Figure 6From: ELF magnetic fluctuations detected by Kaguya in deepest lunar wake associated with type-II protonsWave activity that appeared on field lines disconnected from the lunar surface. Dynamic spectrum of y component B y -sse of magnetic field measured by MAP-LMAG on board Kaguya on 4 April 2008 and particle measurement by MAP-PACE. Format is the same as in Figure 5. Gray dashed lines indicate times of abrupt changes in interplanetary magnetic field.Back to article page