本文采用非径向磁流管位形的假设,计算了太阳冕洞网络部分的色球-日冕过渡区的能量平衡模型。
Energy balance models of the chromosphere-corona transition region are computed for a segment of coronal hole assuming a nonradial magnetic field geometry.
讨论了非平衡B指派问题的求解算法,给出了暂态混沌神经网络模型,并描述了非平衡B指派问题,提出了基于暂态混沌神经网络的非平衡B指派问题的求解算法。
The solution of imbalance B-assignment problem is studied. An assignment's model and network are discussed, and then a new algorithm based on transient chaotic neural networks is proposed.
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