本文用40Cr 钢研究了奥氏体晶粒的异常长大过程以及加热前的原始组织对异常长大过程的影响,并利用已有的计算驱动力 P 及阻力 F 的公式进行了定量计算及分析讨论。结果表明,当奥氏体起始晶粒的 P>F 时,晶粒将发生长大。在长大过程中...本文用40Cr 钢研究了奥氏体晶粒的异常长大过程以及加热前的原始组织对异常长大过程的影响,并利用已有的计算驱动力 P 及阻力 F 的公式进行了定量计算及分析讨论。结果表明,当奥氏体起始晶粒的 P>F 时,晶粒将发生长大。在长大过程中,已开始长大的大晶粒不断吞并周围小晶粒,周围小晶粒则基本上不长大。当小晶粒消失,大晶粒彼此相遇时,长大将终止。可以通过预备热处理调整加热前的原始组织,从而改变奥氏体起始晶粒的 D、D_(n,x)、Z_0及r,控制 P 及 F。对 Zener、Gladman,等的公式进行了校验。结果表明,按戚正风公式计算所得 P 与实测结果符合得最好。按 Zener 公式计算所得 P 偏高,按 Gladmom 公式计算所得 P 又偏低。展开更多
In this paper, a sample including 68 blazars (18 BL Lacs and 50 FSRQs) with known Doppler factors and superluminal velocity from our previous papers is presented. Both the Lorentz factors (/') and viewing angles (...In this paper, a sample including 68 blazars (18 BL Lacs and 50 FSRQs) with known Doppler factors and superluminal velocity from our previous papers is presented. Both the Lorentz factors (/') and viewing angles (0) are estimated for the 68 sources The relationship between BL Lacs and FSRQs is also revisited using the two variables off'and 0. The Lorenz factors are in the range of 2.33 to 64.07. The viewing angles are in the range of 0.04 to 24.56. The averaged value of the viewing angle for BL Lacs is slightly larger than that for FSRQs, while the averaged value of the Lorentz factor for BL Lacs is smaller than that for FSRQs.展开更多
文摘本文用40Cr 钢研究了奥氏体晶粒的异常长大过程以及加热前的原始组织对异常长大过程的影响,并利用已有的计算驱动力 P 及阻力 F 的公式进行了定量计算及分析讨论。结果表明,当奥氏体起始晶粒的 P>F 时,晶粒将发生长大。在长大过程中,已开始长大的大晶粒不断吞并周围小晶粒,周围小晶粒则基本上不长大。当小晶粒消失,大晶粒彼此相遇时,长大将终止。可以通过预备热处理调整加热前的原始组织,从而改变奥氏体起始晶粒的 D、D_(n,x)、Z_0及r,控制 P 及 F。对 Zener、Gladman,等的公式进行了校验。结果表明,按戚正风公式计算所得 P 与实测结果符合得最好。按 Zener 公式计算所得 P 偏高,按 Gladmom 公式计算所得 P 又偏低。
基金supported by the National Natural Science Foundation of China (Grant Nos. 10633010 and 11173009)the National Basic Research Program of China (Grant No. 2007CB 815405)+4 种基金the Bureau of Education of Guangzhou Municipality (Grant No. 11 Sui-Jiao-Ke[2009])Guangdong Province Universities and Colleges Pearl River Scholar Funded Scheme(GDUPS) (2009), Yangcheng Scholar Funded Scheme (Grant No.10A027S)Hunan Provincial Natural Science Foundation of China (Grant No. 10JJ3020)the Fund of the 11th Five-year Plan for Key Construction Academic Subject (Optics) of Hunan Provincethe research fund of Hunan University of Arts and Science (Grant No. JJZD201101)
文摘In this paper, a sample including 68 blazars (18 BL Lacs and 50 FSRQs) with known Doppler factors and superluminal velocity from our previous papers is presented. Both the Lorentz factors (/') and viewing angles (0) are estimated for the 68 sources The relationship between BL Lacs and FSRQs is also revisited using the two variables off'and 0. The Lorenz factors are in the range of 2.33 to 64.07. The viewing angles are in the range of 0.04 to 24.56. The averaged value of the viewing angle for BL Lacs is slightly larger than that for FSRQs, while the averaged value of the Lorentz factor for BL Lacs is smaller than that for FSRQs.
