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Interhemispheric comparison of average substorm onset locations: evidence for deviation from conjugacy

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Figure

Fig. 2. Superposed epoch analysis of solar wind parameters aroundauroral breakup. The key time, “0”, corresponds to the onset time.Parameters from top to bottom are IMFBz, merging electric field,Em, and solar wind density, Np, which have been propagated to
Fig. 3.Number of events of substorm onsets as a function of MLT and MLat for IMF By>0 and IMF By<0 in the Northern (left) andSouthern (right) Hemisphere.
Fig. 4. Same as Fig. 3, but for IMF Bz>0 and Bz<0.
Fig. 5. Same as Fig. 3, but for solar zenith angle, SZA>100◦ (darkness) and SZA<100◦ (sunlight).
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