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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Analysis of the 3–7 October 2000 and 15–24 April 2002 geomagnetic storms with an optimized nonlinear dynamical model
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Analysis of the 3–7 October 2000 and 15–24 April 2002 geomagnetic storms with an optimized nonlinear dynamical model

机译:使用优化的非线性动力学模型分析2000年10月3日至7日和2002年4月15日至24日

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A computationally optimized low-dimensional nonlinear dynamical model of the magnetosphere-ionosphere system called WINDMI is used to analyze two large geomagnetic storm events, 3–7 October 2000 and 15–24 April 2002. These two important storms share common features such as the passage of magnetic clouds, shock events from coronal mass ejections, triggered substorms, and intervals of sawtooth oscillations. The sawtooth oscillations resemble periodic substorms but occur in association with strong or building ring current populations and have injection regions that are unusually close to the Earth and unusually wide in magnetic local times (Henderson et al., 2006; Borovsky et al., 2007). The April 2002 event includes one of the best examples of sawtooth events ever observed. On 18 April 2002, sawtooth oscillations were clearly visible when solar wind conditions (IMF B z , density, pressure) were relatively steady with a slowly varying Dst. In this study, WINDMI is used to model the 3–7 October 2000 and 15–24 April 2002 geomagnetic activity. WINDMI results are evaluated focusing on the sawtooth intervals and the overall prediction of the westward auroral electrojet (AL) index and Dst index. The input to the model is the dynamo driving voltage derived from the fluctuating solar wind plasma and the interplanetary magnetic field measured by the ACE satellite. The output of the model is a field-aligned current proportional to the AL index and the energy stored in the ring current which is proportional to the Dst index. The model parameters are optimized using a genetic algorithm (GA) to obtain solutions that simultaneously have least mean square fit to the AL and Dst indices and also exhibit substorms of period 2–4 hours. The GA optimization results show that the model is able to predict the Dst index reliably and captures the timing and periodicity of the sawtooth signatures in the AL index reasonably well for both storm events.
机译:磁层-电离层系统的一种经过计算优化的低维非线性动力学模型,称为WINDMI,用于分析两个大型地磁风暴事件,即2000年10月3日至7日和2002年4月15日至24日。这两个重要的风暴具有共同的特征,例如通过磁云,日冕物质抛射引起的冲击事件,触发的亚暴以及锯齿波振荡的间隔。锯齿波的振荡类似于周期性的亚暴,但与强的或正在形成的环流种群有关,并且具有注入区域,这些注入区域异常靠近地球并且在磁局部时间异常宽(Henderson等,2006; Borovsky等,2007)。 。 2002年4月的事件包括有史以来最好的锯齿事件之一。 2002年4月18日,当太阳风条件(IMF B z,密度,压力)相对稳定且Dst缓慢变化时,锯齿状振荡清晰可见。在本研究中,WINDMI用于模拟2000年10月3日至7日和2002年4月15日至24日。对WINDMI的结果进行了评估,重点是锯齿间隔以及向西极光电喷(AL)指数和Dst指数的总体预测。该模型的输入是从波动的太阳风等离子体和ACE卫星测得的行星际磁场得出的发电机驱动电压。该模型的输出是与AL指数成比例的场对准电流,以及在环形电流中存储的与Dst指数成比例的能量。使用遗传算法(GA)对模型参数进行优化,以获得同时具有最小均方拟合度AL和Dst指数的解决方案,并且还表现出2-4小时的亚暴风雨。遗传算法的优化结果表明,该模型能够可靠地预测Dst指数,并且对于两种暴风雨事件都能很好地捕获AL指数中的锯齿特征信号的时间和周期性。

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