The southern hemisphere aurora also has differences eg kp index intent really useful, bz numbers are more important instance.The peak of the aurora activity is usually 1 year AFTER the peak of the solar cycle which is measured by the sunspot numbers. That is related to more frequent coronal holes after the sun-spot maximum and the move of the sun-spots to the solar equator over the solar cycle. The effect also depends on the terrestrial latitude with the aurora oval only little affected by this variations while locations further away from it (e.g. central Europe or the mid- and southern US) being more affected.
Given the number X class flares recently, the sun is still pretty active! Just need them pointing more our way and less moonlight
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