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Using ultra-low frequency waves and their characteristics to diagnose key physics of substorm onset

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Figure

Fig. 1 Locations of the ground magnetometers from the CARISMA, THEMIS, CANMOS and McMAC magnetometer chains (for details see text)
Fig. 2 North–south slices (keograms) from the GILL THEMIS ASI and GILL NORSTAR MSP from 05:30:30 to 06:30:30 UT
Fig. 3 AWESOME (Murphy et al. ficients, whereby black represents wavelet coefficients below the pre-determined threshold for each j and yellow-orange-red-white are coefficients 2009a) analysis of the substorm in 2008-03-05/06:04:20 UT, run from 05:55:00 UT
Figure b shows the relative timing between the Pi1-2 lated below 55° latitude since the Pi1 onsets were only observed over a limited spatial region

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