This analysis reveals a unique shock-substorm onset in 1998, suggesting new insights into substorm dynamics.
An interplanetary shock triggered a substorm with a peak intensity SML = −1,781 nT on 24 September 1998. This is called a shock‐substorm here to differentiate it from generic substorms. The shock, with a speed of ∼790 km s −1 , caused the release of prestored magnetosphere/magnetotail energy plus additional solar wind input energy, the latter unusual for a shock‐nonsupersubstorm event. The internal magnetospheric shock/wave had a speed of ∼630 km s −1 , consistent with arriving at x = −6 R E at the time of substorm onset. The internal shock arrival to x = −10 R E would have been after the substorm onset time, so magnetic reconnection for the substorm triggering can be ruled out. Akasofu (2023, https://doi.org/10.1093/mnras/stac3187 ) has stated that there are many different types of substorm onsets. We believe that this shock‐substorm is different than generic substorms.
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Tsurutani et al. (2025) studied this question.
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