首页> 外文会议>Second Solar Cycle and Space Weather Euroconference Sep 24-29, 2001 Vico Equense, Italy >NEURAL NETWORK PREDICTION OF SOLAR PROTON EVENTS WITH LONG LEAD TIMES
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NEURAL NETWORK PREDICTION OF SOLAR PROTON EVENTS WITH LONG LEAD TIMES

机译:铅时间长的质子事件的神经网络预测

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The high-energy particles that are emitted by the sun during Solar Proton Events (SPEs) pose a serious hazard to interplanetary and near-earth spacecraft causing damage to electronics, spurious signals and a general disruption of spacecraft operations. An analysis of GOES x-rays and full disk solar radio flux prior to proton events has revealed significant differences compared to times at which no proton events occurred. Selecting predictor variables using the F-statistic, neural network models have been generated which use data from tens of days prior to SPEs to predict their occurrence 48 hours in advance with a 65% success rate. This is an improvement in lead time of an order of magnitude over current SPE prediction models.
机译:太阳在质子事件(SPE)中散发出来的高能粒子会对行星际和近地航天器造成严重危害,从而损坏电子设备,虚假信号并严重干扰航天器的运行。对质子事件之前的GOES X射线和全盘太阳辐射通量的分析显示,与没有质子事件发生的时间相比,存在显着差异。使用F统计量选择预测变量,已经生成了神经网络模型,该模型使用SPE之前数十天的数据提前48小时预测其发生,成功率为65%。这比当前的SPE预测模型将交货时间缩短了一个数量级。

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