Optical Flash of GRB 990123: Constraints on the Physical Parameters of the Reverse Shock     

Yi-Zhong Fan  Zi-Gao Dai  Yong-Feng Huang  Tan Lu Department of Astronomy  Nanjing University  Nanjing 《中国天文和天体物理学报》2002,2(5):449-453

The optical flash accompanying GRB 990123 is believed to be powered by the reverse shock of a thin shell. With the best-fit physical parameters for GRB 990123 and the assumption that the parameters in the optical flash are the same as in the afterglow, we show that: 1) the shell is thick rather than thin, and we have provided the light curve for the thick shell case which coincides with the observation; 2) the theoretical peak flux of the optical flash accounts for only 3×10~-4 of the observed. In order to remove this discrepancy, the physical parameters, the electron energy and magnetic ratios, εe and εB, should be 0.61 and 0.39, which are very different from their values for the late afterglow.  相似文献   

黄土土性的空间自相关性研究     

倪万魁  牛富俊  刘东燕 《地球科学与环境学报》2002,24(2):4-8

运用土层的随机场模型研究了绛帐、潼关和延安黄土主要物理力学指标沿深度的统计规律,计算出黄土土性的自相关距离,探讨了黄土土性的空间变异性,结果认为:黄土的物理力学指标沿深度均是统计非均匀的,在实际工程的设计中,如果把土层看成统计均匀,其土性参数的标准差会比实际情况大,从而会导致较大的误差。  相似文献   

Rhombic Cell Analysis. Ⅱ. Application to the IRAS／PSCz Catalogue     

Tao Kiang  Yong-Feng Wu  Xing-Fen Zhu Dunsink Observatory Dublin Institute for Advanced Studies Dublin Ireland Center for Astrophysics  University of Science  Technology of China  Hefei 《中国天文和天体物理学报》2004,4(3):209-220

Rhombic cell analysis as outlined in the first paper of the present seriesis applied to samples of varying depths and liming luminosities of the IRAS/PSCzCatalogue. Numerical indices are introduced to summarize essential information.Because of the discrete nature of the analysis and of the space distribution of galax-ies, the indices for a given sample must be regarded as each having an irreduciblescatter. Despite the scatter, the mean indices show remarkable variations acrossthe samples. The underlying factor for the variations is shown to be the limitingluminosity rather than the sampling depth. As samples of more and more luminousgalaxies are considered over a range of some 2.5 magnitudes (a factor of some 75in space density), the morphology of the filled and empty regions defined by thegalaxies degrades steadily towards insignificance, and the degrading is faster for thefilled than the empty region.  相似文献   

黑宝山─木耳气煤盆地含煤建造的垂向层序与旋回特征     

王喜臣  白昶生 《黑龙江地质》1992,3(4):32-37

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结构计算的地震荷载模型     

д.  ВМ 李锟 《世界地震工程》1989,(1):50-52,58

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高频VLBI观测射电源的结构     

田文武  张海燕等 《云南天文台台刊》2001,(2):1-9

高频VLBI观测揭示出河外射电源在pc或者亚pc尺度上大都有核-喷流的内部结构，尤其是对平谱致密射电源中毫角秒尺度的子源，能以相当高的概率观测到它的视超光速现象。多频观测可监测到一些新喷流子源的出现，特别在射电激变源中这些新喷流子源的出现与宽带内（从光学到γ射线）的爆发相关。且得到的一些源的核区谱指数分布，为确认源的VLBI核提供了支持。  相似文献   

维护农民合法权益促进农民增加收入     

杨任远 《江苏国土资源》2002,(2):5-7

国土资源部门是涉农部门。土地是农民的命根子，为“三农”服务特别是维护农民土地权益、促进农民增收，是国土资源部门义不容辞的职责。回顾总结了近年来这方面的工作，指出了今后一个时期国土资源部门为“三农”服务的方向。  相似文献   

地震危险性敏感分析：一种多参数方法     

Rabin.  N 王健 《世界地震译丛》1993,(2):30-30,34,45

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大气参数变化对VLBI对流层时延计算值的影响     

杨志根 《中国科学院上海天文台年刊》1993,(14):238-242

本采用我国上海、昆明和乌鲁木齐三个VLBI站的对流层大气高度参数ht和对流层内温度垂直梯度βt参数月均值资料，估计了对干大气时延的影响，结果表明在地平高度ε＝10°－20°时两参数的变化可引起干大气时延周年变化的幅值分别为1-5mm和2-15mm；ht的周日变化也可引起大气时延周日变化约1mm，因此，对于1ps级精度的VLBI物理模型，ht和βt不应当采用测站的固定常数值。  相似文献   

Comparison of Taste Components between Triploid and Diploid Oyster     

LINHong WANGXiaoxue ZHANGBin TANGHaiqing XUEChanghu XUJiachao 《青岛海洋大学学报(英文版)》2002,1(1):55-58

The main taste components of triploid and diploid oyster (Crassostrea gigas) were compared. Free amino acids, inosine monophosphate, succinate, trimethylamine oxide and betaine in fresh and boiled extractives were analyzed. The protein, lipids, glycogen, moisture and ash, which may affect the flavour, were evaluated. In boiled extractives, the amino acids were 394.1 mg(100g)^-1 in diploid and 183.5 mg(100g)^-1 in triploid. However, in fresh oyster extractives, they were 320.0 mg(100g)^-1 and 147.3 mg(100g)^-1 respectively. The inosine monophosphate in triploid was 44% more than that in diploid, and a little difference existed in the content of trimethylamine oxide between them. The contents of these taste components were the basis for taste flavour pattern determination.  相似文献