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Solar particle event dose prediction using kernel regression

机译:使用核回归的太阳粒子事件剂量预测

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Solar energetic particle events (SEPs) are a naturally occurring phenomenon in which subatomic particles are radiated from the sun. Astronauts in deep space could be subjected to significant radiation exposures due to these events. The dose is usually received over approximately a 20–40 hour interval. The effects of these particles could be mitigated by an early detection and warning system, which provides reliable estimates of the magnitude of the expected radiation dose from the event. For this purpose we have created a new software package designed to forecast the final total dose for the event, from doses measured early in the event cycle. This package implements a sliding scale kernel regression model to calculate an estimate for the projected total dose. The software displays a plot of both the current dose forecast and a history of previous predictions. These predictions are accompanied by uncertainty estimates. Sample results are presented.
机译:太阳高能粒子事件(SEP)是自然发生的现象,其中亚原子粒子从太阳辐射出来。由于这些事件,深太空中的宇航员可能会遭受大量的辐射暴露。通常在大约20-40小时的间隔内接受剂量。这些粒子的影响可以通过早期检测和预警系统来减轻,该系统可以提供对该事件的预期辐射剂量大小的可靠估计。为此,我们创建了一个新的软件包,旨在根据事件周期早期测量的剂量来预测事件的最终总剂量。该软件包实现了滑动比例内核回归模型,以计算预计总剂量的估计值。该软件会显示当前剂量预测和先前预测历史的图。这些预测伴随着不确定性估计。给出了样本结果。

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