通海台垂直摆受建筑载荷影响的数值模拟研究     

岳冲  李利波  闫伟  洪敏 《大地测量与地球动力学》2022,42(9):985-990

针对通海台垂直摆NS和EW测项自2019-04出现同步趋势转折变化,计算2017~2020年NS和EW测项M₂波潮汐因子。结合监测井等地下介质结构资料,构建通海台沿垂向分层的三维有限元物理模型,定量分析不同岩石参数模型下建筑载荷对通海台NS向及EW向位移影响的差异特征。结果表明：1）2019-04后NS测项N倾变化量达到约2 750 ms,而EW测项E倾变化量达到约580 ms,NS测项趋势变化量显著大于EW测项;2）2017~2020年NS和EW测项M₂波潮汐因子较为稳定,NS测项M₂波潮汐因子在0.7左右波动,EW测项M₂波潮汐因子在0.52左右波动,数据的转折变化未能在潮汐频段引起同步变化;3）位于通海台东北部的医院建筑物载荷在通海台附近产生N向和E向位移加载,与垂直摆NS和EW测项在2019-04后出现的N倾和E倾趋势转折变化较为一致,模拟得到的N向位移量约为E向位移量的3倍。  相似文献   

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κ���  ��һ��  �ս��� 《大地测量与地球动力学》2014,34(5):17-20

??????M8.0????????????????????С???????????????????о???????????λ????????????????????ν???ие???????????????????1??M8.0??????????????????????????????????????С????????????????????????????????????????????????42°????????????????????????????20 km??2?????????????????????????????????????10 km?????????????????С??????????????????????????????????????????????????????λ?????????7 km??3??2??14??
ML3.7?????????????????93°?????????????????????С??????????????????????????????????2???????￡????????????????????????????????????????????????????????????????4??2??28??ML3.8?????????λ?????????????????????????????????????????????????????????￡????????????  相似文献   

计算机图像处理在增强华县地震构造遥感信息中的应用     

范秋林 《大地测量与地球动力学》1994,(1)

由于地震构造的许多重要信息在卫片上显示往往比较隐晦，必须对其进行增强处理，以取得最佳的解译效果。本文以历史上曾发生过八级地震的华县地震构造带为例，讨论辐射增强、多波段频谱变换、空间变换假彩色增强、分类等计算机图象处理方法的若干功能，以及这些功能在不同背景条件下的处理效果，为分析该地区活动断裂、地质构造等提供了有意义的信息，也为这种处理手段在地震构造信息分析等方面的推广应用提供参考。  相似文献   

Intermediate mass black holes in accreting binaries: formation, evolution and observational appearance     

Simon F. Portegies Zwart  Jasinta Dewi  Tom Maccarone 《Monthly notices of the Royal Astronomical Society》2004,355(2):413-423

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我国应建立测绘监理制度     

王威 《地理信息世界》2002,(1)

测绘监理是依据测绘行政法规和技术标准 ,综合运用法律、经济、行政、技术标准和有关政策 ,为确保测绘行为的合法性和科学性对测绘项目所进行的全过程有效监控。建立一套符合中国国情的测绘工程监理制度 ,对我国的测绘行政管理具有十分重要的意义  相似文献   

A SAURON study of M32: measuring the intrinsic flattening and the central black hole mass     

E. K. Verolme  M. Cappellari  Y. Copin  R. P. van der Marel  R. Bacon  M. Bureau    R. L. Davies  B. M. Miller  P. T. de Zeeuw 《Monthly notices of the Royal Astronomical Society》2002,335(3):517-525

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Global very long-baseline interferometry observations of compact radio sources in M82     

A. R. McDonald  T. W. B. Muxlow  A. Pedlar  M. A. Garrett  K. A. Wills  S. T. Garrington  P. J. Diamond  P. N. Wilkinson 《Monthly notices of the Royal Astronomical Society》2001,322(1):100-106

Observations of the starburst galaxy, M82, have been made with a 20-station global very long-baseline interferometry (VLBI) array at λ 18 cm. Maps are presented of the brightest young supernova remnants (SNR) in M82 and the wide-field mapping techniques used in making images over a field of view of ∼1 arcmin with 3-milliarcsecond resolution are discussed. A limit has been placed on the power-law deceleration of the young supernova remnant (SNR) 43.31+592 with an index greater than 0.73±0.11 from observations with the European VLBI Network. Using the global array we have resolved compact knots of radio emission in the source which, with future global observations, will enable better constraints to be placed on the expansion parameters of this SNR.
The latest global observations have also provided high-resolution images of the most compact radio source in M82, 41.95+575. We determine an upper limit to the radial expansion rate along the major axis of 2000 km s⁻¹. However, the new images also show structure resembling that of collimated ejection which brings into question the previous explanation of the source as being a result of the confinement of a supernova by a high-density circumstellar medium.
It is apparent that we are now able to image the brightest supernova remnants in M82 with a linear scale which allows direct comparison with galactic SNR such as Cassiopeia A.  相似文献   

The short-period supersoft source in M31     

A. R. King  J. P. Osborne  K. Schenker 《Monthly notices of the Royal Astronomical Society》2002,329(2):L43-L46

We show that the recently discovered short period supersoft source in M31 is probably a progenitor of a magnetic cataclysmic variable (CV). The white dwarf spins asynchronously because of the current high accretion rate. However its fieldstrength is typical of an AM Herculis system, which is what it will ultimately become. We discuss the relevance of this system to CV evolution, and its relation to some particular CVs with special characteristics.  相似文献   

Chemical abundances of planetary nebulae from optical recombination lines – III. The Galactic bulge PN M 1-42 and M 2-36     

X.-W. Liu  S.-G. Luo  M.J. Barlow  I.J. Danziger  P.J. Storey 《Monthly notices of the Royal Astronomical Society》2001,327(1):141-168

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Hydrodynamics of photoionized columns in the Eagle Nebula, M 16     

R.J.R. Williams  D. Ward-Thompson  A.P. Whitworth 《Monthly notices of the Royal Astronomical Society》2001,327(3):788-798

We present hydrodynamical simulations of the formation, structure and evolution of photoionized columns, with parameters based on those observed in the Eagle Nebula. On the basis of these simulations we argue that there is no unequivocal evidence that the dense neutral clumps at heads of the columns were cores in the pre-existing molecular cloud. In our simulations, a variety of initial conditions leads to the formation and maintenance of near-equilibrium columns. Therefore, it is likely that narrow columns will often occur in regions with large-scale inhomogeneities, but that observations of such columns can tell us little about the processes by which they formed. The manner in which the columns in our simulations develop suggests that their evolution may result in extended sequences of radiation-induced star formation.  相似文献