The effect of non-hydrostatic pressure distribution downstream of the shock front is taken into account.
所有这些计算都考虑了波后非静水压力分布的影响。
The artificial viscosity can control the oscillations trailing the shock front, but it also weakened the peak pressure.
人工粘性能够较好地抑制冲击波压力计算中出现的数值振荡,但同时也引起了冲击波峰值的衰减。
Its strong stellar wind precedes it, compressing and heating the dusty interstellar material and shaping the curved shock front.
强烈的恒星风压缩加热了星际尘埃,并在前方形成弧形的震荡波。
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