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Reasons why some solar wind changes do not trigger substorms

机译:为什么一些太阳风的变化不触发亚暴的

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Previous studies have shown that a northward turning of the interplanetary magnetic field (IMF) or a reduction in the magnitude of IMF B y component can trigger a substorm. Also a solar wind dynamic pressure enhancement has been found to trigger a substorm under strongly southward IMF conditions. Solar wind changes directed opposite to those of, or not satisfying the conditions of, these known triggers may be considered as inherently nontriggers. In the present paper we have examined 12 events where more than one solar wind quantity change simultaneously and no substorm is triggered. We suggest that nontriggering by the solar wind changes studied in the present work can be explained by the following three reasons: (1) there is a lack of, or insufficient, substorm growth phase development prior to the potential triggering change; (2) the solar wind change is an inherently nontriggering change; (3) the nullifying effect occurs, where one quantity changes in the direction of a substorm trigger and simultaneously another quantity changes in the direction opposite to that of a trigger. The nontriggering types found in this study are consistent with the suggestion that variations of the solar wind that do not reduce the convection strength within the inner plasma sheet do not trigger substorms, which is opposite to what is expected from a triggering solar wind variation.
机译:之前的研究表明,向北行星际磁场的转变(国际货币基金组织(IMF)或减少国际货币基金组织B的大小y组件可以引发亚暴。风动态压力增强被发现引发强烈向南下亚暴国际货币基金组织的条件。相反的,或不满足条件,这些已知的诱因视为天生nontriggers。本文中,我们介绍了12活动不止一个太阳风数量变化同时不引发亚暴。建议由太阳风nontriggering在目前的研究工作可以变化解释以下三个原因:(1)有一个缺乏或不足,亚暴前成长阶段发展的潜力触发变化;一个天生nontriggering变化;取消效应发生时,其中一个量亚暴触发的方向变化同时另一个量的变化方向相反的触发器。本研究中发现的nontriggering类型与建议的变化一致不会减少对流的太阳风在内部等离子体片不力量什么是触发为亚暴,是相反的预计从引发太阳风的变化。

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