Bruce T. Tsurutani, Rajkumar Hajra, Yusuke Ebihara, Gurbax S. Lakhina, Yasuhito Narita, Karl-Heinz Glassmeier
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引用次数: 0
摘要
1998年9月24日,一次行星际激波引发了一次峰值强度为SML =−1781 nT的亚暴。这里称之为冲击亚暴以区别于一般的亚暴。激波的速度约为790 km / s−1,导致预先储存的磁层/磁尾能量和额外的太阳风输入能量的释放,后者在激波-非超级亚暴事件中是不寻常的。内部磁层激波的速度为~ 630 km s−1,与亚暴发生时到达x =−6 RE的速度一致。内部冲击到达x =−10 RE将是在亚暴开始时间之后,因此可以排除触发亚暴的磁重联。Akasofu (2023, https://doi.org/10.1093/mnras/stac3187)指出,有许多不同类型的次暴爆发。我们认为这次冲击亚暴不同于一般的亚暴。
The Shock-Substorm of 24 September 1998: A Different Type of Substorm Trigger Onset
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 RE at the time of substorm onset. The internal shock arrival to x = −10 RE 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.
期刊介绍:
Geophysical Research Letters (GRL) publishes high-impact, innovative, and timely research on major scientific advances in all the major geoscience disciplines. Papers are communications-length articles and should have broad and immediate implications in their discipline or across the geosciences. GRLmaintains the fastest turn-around of all high-impact publications in the geosciences and works closely with authors to ensure broad visibility of top papers.