半无限空间中SH波被空腔和刚性包体所散射(英文)     

曾心传  A.S.Cakmak 《大地测量与地球动力学》1985,(3)

根据波尔近似,借助于波动积分方程,近似求解半无限弹性空间中平面SH波由圆形空腔和刚性包体所散射的问题。获得了空腔表面上的散射位移、作用于被包体上的剪应力、半空间表面形变以及远场位移的近似公式。在数值计算中,ka(k=波数,a=空腔或被包体的半径)取为1.0,γ(SH波的入射角,从垂向方向起算)取为π/4。  相似文献   

加拿大萨斯喀彻温铀矿勘查和开发进展（1992—1993年）     

戴杰敏  李月祥 《国外铀金地质》1995,12(4):316-318

加拿大萨斯喀彻温的铀储量和产量在世界上占有重要地位，目前已探明的铀储量约４０００００ｔ铀生产量约８５００ｔ／ａ。近年的勘查无重要的世界级发现。麦克阿瑟河的Ｐ２Ｎ矿床储量由７７０００ｔ增加到１０００００ｔ，而伊格尔岬矿床的储量则由４７０００ｔ减少为２５０００ｔ。由于国际铀市场疲软，勘查投入削减，但仍在继续，铀矿开发也在加快，麦克阿瑟河Ｐ２Ｎ、伊格尔岬，麦克莱恩湖，西茄湖、中西湖和克拉夫湖等矿床将先后  相似文献   

A NEW“TETRASPORANGIAL”SPECIES OF LIAGORA(RHODOPHYTA,NEMALIALES)FROM HAWAIT     

Isabella A. Abbott 《中国海洋湖沼学报》1995,(4)

A new species of Liagora,L.perennis sp.nov.from Hawai’i,is described.Unlike dpecies of this genus in China,it is carpotetrasporangial,and at the place of expected carposporangia bears cruciately di-vided tetrasporangia,a detail which differentiates it from the usual species of Liagora without tetraspores that have been reported in China.Notes are provided on other Liagora species that have an impact on the taxonomy of species found in China.  相似文献   

首都圈地区现今断层活动的数学模拟及地震危险性讨论     

李群芳  张云柱  高忠宁 《大地测量与地球动力学》1995,(1)

以首都圈地区现今活动断层上近２０年的位移测量资料为依据，用二维线弹性有限元对该区断层的活动特征进行了拟合，并结合有关资料讨论了该区的地震危险性。结果表明：１９７７－１９８６年间该区主压应力优势方位与华北较一致，约为Ｎ４５°－８０°Ｅ；１９８６－１９９０年其主压应力方向向北偏转，约为Ｎ５°－６０°Ｅ；１９９０年至现在其主压应力又向东偏转，角度大于第一阶段，约为Ｎ８０°－９５°Ｅ。该区的张家口－延庆一带近期有发生中强震的可能；丰镇－阳高－大同地区和凉城－古营盘地区应力较高，也应引起注意。  相似文献   

Identification of the interstellar cyanomethyl radical (CH2CN) in the molecular clouds TMC-1 and Sagittarius B2     

Irvine WM  Friberg P  Hjalmarson A  Ishikawa S  Kaifu N  Kawaguchi K  Madden SC  Matthews HE  Ohishi M  Saito S  Suzuki H  Thaddeus P  Turner BE  Yamamoto S  Ziurys LM 《The Astrophysical journal》1988,334(2):L107-L111

We report the astronomical identification of the cyanomethyl radical, CH2CN, the heaviest nonlinear molecular radical to be identified in interstellar clouds. The complex fine and hyperfine structures of the lowest rotational transitions at about 20.12 and 40.24 GHz are resolved in TMC-1, where the abundance appears to be about 5 x 10(-9) relative to that of H2. This is significantly greater than the observed abundance of CH3CN (methyl cyanide) in TMC-1. In Sgr B2 the hyperfine structure is blended in the higher frequency transitions at 40, 80, and 100 GHz, although the spin-rotation doubling is clearly evident. Preliminary searches in other sources indicate that the distribution of CH2CN is similar to that for such carbon chain species as HC3N or C4H.  相似文献   

The possible formation of a hydrogen coma around comets at large heliocentric distances     

Bar-Nun A  Prialnik D 《The Astrophysical journal》1988,324(1):L31-L34

An observational test--the detection of a hydrogen coma around comets at large heliocentric distances--is proposed for determining whether comets were formed by the agglomeration of unaltered, ice-coated, interstellar grains. Laboratory experiments showed that amorphous water ice traps H2, D2, and Ne below 20 K and does not release them completely until the ice is heated to 150 K. Gas/ice ratios as high as 0.63 are obtainable. Thus, if the ice-coated interstellar grains were not heated above approximately 110 K, prior to their agglomeration into cometary nuclei, the inward propagating heat waves should release from the comets a continuous flux of molecular hydrogen. This flux would exceed that of water molecules at approximately 3 AU preperihelion and approximately 4 AU postperihelion.  相似文献   

Variations in the HCN/HNC abundance ratio in the Orion molecular cloud     

Goldsmith PF  Irvine WM  Hjalmarson A  Elldér J 《The Astrophysical journal》1986,310(1):383-391

We have used observations of the rare isotopes of HCN and HNC to determine the relative abundance of these two chemical isomers along the central ridge of the Orion molecular cloud. The abundance ratio [HCN]/[HNC] decreases by more than an order of magnitude from the relatively warm plateau and hot core sources toward the KL nebula to the colder, more quiescent clouds to the north and south. Even in the cooler regions, however, the ratio is an order of magnitude larger than that found in previous investigations of cold dark clouds. We determine the kinetic temperature in the regions we have studied from new observations of methylacetylene (CH3CCH), together with other recent estimates of the gas temperature near KL. The results suggest that the warmer portions of the cloud are dominated by different chemical pathways than those in the general interstellar cloud material.  相似文献   

高能偏振能量色散X射线荧光光谱仪应用现状和进展   总被引：4，自引：2，他引：2  

吉昂  李国会  张华 《岩矿测试》2008,27(6):451-462

对高能偏振能量色散X射线荧光光谱仪基本特点及其用于环境、生物、地质样品中痕量元素的分析和RoSH检测等领域的应用现状予以介绍,并对二次靶与滤光片在痕量元素分析中的应用作了探讨。  相似文献   

跨孔电阻率法有限元数值模拟及反演     

李天成  牛滨华  孙春岩  慕洪涛 《地质与勘探》2008,44(3):52-55

油气资源和矿产资源勘探中,常需要较大的勘探深度和较高的深部分辨能力.充分利用现有钻孔的井地或跨孔电阻率成像技术适应这种要求,但引起的视电阻率响应复杂,从而给资料的正确处理与解释带来一定的困难,为此有必要通过正演数值模拟和反演相结合的手段,对理论模型井地或跨孔装置的响应异常规律进行研究.文章通过设计一个典型地质模型,利用Ansys有限元软件对模型进行2D跨孔电阻率法有限元正演计算,并将模拟的响应视电阻率作为反演的输入,结合平滑约束最小二乘反演,分析了异常特征和分布规律.  相似文献   

Geological research at the Natural History Museum of Moscow University, 1759-1930 （in Russian）     

Zoya A. Bessudnova 《《幕》》2008,31(3):368-369

In 2006, the Moscow publishing house Nauka （Science） published a 246-page book by Zoya A. Bessudnova entitled Geological Research at the Natural History. Museum of Moscow University, 1759-1930 as No. 32 in its series ＂Sketches on the History of Geological Knowledge＇. The author is a geologist and Senior Researcher in the Department for the History of Geology of the Vernadsky State Geological Museum of the Russian Academy of Sciences, and a member of the International Commission on the History of Geological Sci- ences （INHIGEO）.  相似文献