漂移壳追踪方法与内辐射带的长期变化

地磁场的长期变化发迹辐射带结构,如何在当前年代下恰当地使用ＡＥ－８／ＡＰ－８模型,目前国内外对此问题存在着很大的争议。我们在物理分析的基础上给出了当前年代下使用辐射带模型ＡＰ－８的漂移壳追踪方法ＤＳＴＭ（Ｄｒｉｆｔ Ｓｈｅｌｌ Ｔｒａｃｉｎｇ Ｍｅｔｈｏｄ）。计算结果表明地磁场的长期变化对内辐射带的通量分布有着显著的影响。３０－４０年来,南大西洋通量异常区中心向丁和向北发生偏移,高粒子辐射区域的范     

Improvement on shaped-hole film cooling effectiveness by integrating upstream sand-dune-shaped ramps

A numerical investigation and experimental validation is performed to address deeper insights into the combined effect of shaped holes and Sand-Dune-shaped upstream Ramp (SDR) on enhancing the film cooling effectiveness, under a wide blowing ratio range (M = 0.25–1.5). Three kinds of holes (Cylindrical Hole (CH), Fan-Shaped Hole (FSH), and Crater-Shaped Hole (CSH)) are taken into consideration. The SDR shows an inherent affecting mechanism on the mutual interaction of jet-in-crossflow. It aggravates the lateral spreading of cooling jet and thus improves the film cooling uniformity significantly, regardless of film-hole shape and blowing ratio. When the blowing ratio is beyond 1.0, the combined effect of shaped holes and SDR on improving film cooling effectiveness behaves more significantly. It is suggested that FSH-SDR is a most favorable film cooling scheme. For FSH-SDR case, the spatially-averaged film cooling effectiveness is increased monotonously with the increase of blowing ratio, among the present bowing ratio range.