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Based on multi-fluid volume fraction and piecewise parabolic method
(PPM), a multi-viscosity-fluid hydrodynamic code MVPPM
(Multi-Viscosity-Fluid Piecewise Parabolic Method) is developed and
applied to the problems of shock-induced hydrodynamic interfacial
instability and mixing. Simulations of gas/liquid interface
instability show that the influences of initial perturbations on the
fluid mixing zone (FMZ) growth are significant, especially at the
late stages, while grids have only a slight effect on the FMZ width,
when the interface is impulsively accelerated by a shock wave
passing through it. A numerical study of the hydrodynamic
interfacial instability and mixing of gaseous flows impacted by
re-shocks is presented. It reveals that the numerical results are in
good agreement with the experimental results and the mixing growth
rate strongly depends on initial conditions. Ultimately, the jelly
layer experiment relevant to the instability impacted by exploding
is simulated. The shape of jelly interface, position of front face
of jelly layer, crest and trough of perturbation versus time are
given; their simulated results are in good agreement with
experimental results. 相似文献
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Accurate and rapid error estimation on global gravitational field from current GRACE and future GRACE Follow-On missions 总被引:10,自引:0,他引:10 下载免费PDF全文
Firstly, the new combined error model of cumulative geoid height
influenced by four error sources, including the inter-satellite range-rate
of an interferometric laser (K-band) ranging system, the orbital
position and velocity of a global positioning system (GPS) receiver
and non-conservative force of an accelerometer, is established from the
perspectives of the power spectrum principle in physics using the
semi-analytical approach. Secondly, the accuracy of the global
gravitational field is accurately and rapidly estimated based on the
combined error model; the cumulative geoid height error is 1.985×
10-1~m at degree 120 based on GRACE Level 1B measured
observation errors of the year 2007 published by the US Jet
Propulsion Laboratory (JPL), and the cumulative geoid height error is
5.825× 10^ - 2~m at degree 360 using GRACE Follow-On
orbital altitude 250~km and inter-satellite range 50 km. The
matching relationship of accuracy indexes from GRACE Follow-On key
payloads is brought forward, and the dependability of the combined error
model is validated. Finally, the feasibility of high-accuracy and
high-resolution global gravitational field estimation from GRACE
Follow-On is demonstrated based on different satellite orbital
altitudes. 相似文献
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空间碎片与航天器的撞击速度通常大于10 km/s,这种速度条件下撞击过程的物理特点是高温、高压和高应变率,同时伴随着熔化、汽化及等离子体等相变问题发生。利用AUTODYN/SPH的二次开发功能,在程序中嵌入Sesame状态方程数据库和铝材料的相图,数值模拟出撞击速度为5.0和5.6 km/s时的防护屏穿孔直径分别为9.02 mm和9.34 mm,计算结果与实验结果符合较好,说明物理建模及参数的选取合理,同时也验证了数值模拟方法的正确性及有效性。通过计算给出碎片云的热力学量压力和温度分布,结合铝的相图,对超高速撞击产生碎片云的相分布进行了初步计算,给出了碎片云中固、液、气相的分布范围。 相似文献
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研究了闪光X射线辐射照像蒙特卡罗程序(FXRMC)在MPI平台下的并行计算实现,给出了实现过程中并行随机数的产生方法。对并行程序的测试结果表明:并行程序与串行程序结果一致,加速比比较理想,呈线性增长,并行效率在16个处理器上可达80%以上。算例的结果说明了并行化可有效地解决程序计算散射技术性能时的耗时问题,从而有效化解FXRMC耗时和大规模计算的困难,提高了FXRMC程序的计算规模和计算速度,达到了研究要求。 (Institute of Fluid Physics, CAEP, P. O. Box 919-105, Mianyang 621900, China) 相似文献
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目的旨在研究四氧化三铁纳米颗粒在大鼠脑积水模型中的磁共振及CT成像中的应用,为临床应用提供理论依据,为合理开发该纳米颗粒奠定实验基础。方法采用单纯随机分组法将60只分为空白对照组(20只,给予无菌生理盐水注入枕大池)和实验组(40只,利用高岭土制作大鼠脑积水模型,利用MR筛选大鼠脑积水模型,向模型蛛网膜下腔内注入四氧化三铁纳米颗粒,1h后行CT检查,并于1个月后在显微镜下观察空白对照组与实验组四氧化三铁纳米颗粒在脑、心、肝、脾肺、肾等器官蓄积情况。结果 (1)实验组手术和麻醉导致6只大鼠死亡,实验组死亡率15%。对照组死亡率10%。总死亡率为13.3%。(2)实验组32只大鼠形成脑积水,在存活大鼠中模型成功率为88.9%,模型总制作成功率80.0%。(3)四氧化三铁在大鼠椎管磁共振成像中显示欠佳,CT具有较好的对比效果;(4)蛛网膜下腔内注入四氧化三铁纳米颗粒1个月后在脑、肝、脾、肺、肾等器官无明显蓄积。结论椎管内注入超磁性四氧化三铁纳米颗粒是安全可靠的,可以作为脑积水颅脑CT检查的造影剂。 相似文献
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