基于岩体塑性位错理论的龙门山区域构造系统演化过程

青藏高原对四川盆地的挤压作用导致了龙门山断裂带的形成及其山脉的隆起。本文以龙门山附近区域板块运动以及深部岩体力学特性为背景,采用FLAC3D软件模拟再现了时间跨度为700万年的龙门山区域构造系统演化过程。研究结果表明:在板块运动作用下,F1、F2和F3断层依次形成,贯通的断层对地表的抬升具有较强的控制作用,当断层贯通于地表后,龙门山及其以西的川西高原持续隆起,平均抬升速率约为1.38mm/yr,而龙门山断裂带以东的川西坳陷只有较小的抬升量,从而导致川西高原抬升8996 m,致使该区域产生6000m左右的落差,模拟的地形特征与目前的龙门山地形地貌基本相似。依据模拟结果与实测资料,绘制了龙门山断裂带形成及其附近区域地形地貌的演化过程图,呈现了板块挤压、断层塑性位错、地表侵蚀和沉积作用等因素共同作用对地形地貌的塑造过程。     

Simultaneous monochromatic and spectral observations of two large loop prominence groups

Using the solar tower telescope of Nanjing University, we observed the two large loop prominence groups of 1982 Dec. 20 and 1983 Feb. 9. Hα photographs and spectra around the Hα and H and K lines were obtained simultaneously. From these data, we derived a line of sight velocity distribution, which agrees perfectly with the distribution for matter falling freely without viscosity. From the widths of the Hα and the K lines, we found the loop material to have a uniform kinetic temperature and a turbulent velocity that increases with height. From the central intensities of the lines we derived a density of n(H) ? 1.3 ? 2.6 × 10¹⁰cm^?3. A possible mechanism of the formation of loop prominence groups and their relation with flares are discussed.     

Rapid reversals of polarization in spikes and fast fine structures

We briefly describe the polarization state of the spike groups and fast fine structures superimposed on the 47GB microwave burst of 1991 May 16. At two frequencies 100 MHz apart, namely, 2645 and 2545 MHz, the polarization showed rapid reversals on short time scales of the order of 50 100ms. We think this is probably related to fluctuations on both short time and small spatial scales, in the plasma density and magnetic field of the emission region. Thése oscillations cause the plasma and cyclotron frequency ratio to vary around the value of , thus making the electron cyclotron maser instability growth rate to be dominated alternately by the X mode and the O mode and the polarization state to switch from one sign to the other.     

Combined radiation mechanism in the sun's active region No. 75 during the eclipse of 16 February, 1980

We assume that the physical conditions above an active solar region vary continuously from the centers of sunspots to the adjacent quiet region and try to take into account the influence of the magnetic field. Thus we calculate the three-dimensional distribution of the electron temperature and density based on the radio spectrum of active region No. 75 obtained from the solar eclipse observation of 16 February, 1980. If we assume a potential field, we calculated the magnetic field above the active region in terms of the solar photospheric magnetic field.Using the electron temperature, density, and the magnetic field as described above, and assuming the slowly varying radiation mechanism to consist of bremsstrahlung and gyro-resonance radiation, we obtained the flux density spectrum and the brightness temperature spectrum. The calculated results are essentially consistent with the observations.     

应用商用CCD配备录像机进行天体定位的试验

本工作是为今后在1.2米望远镜上利用商用CCD配备录像机进行人卫快速精密定位观测所做的初步试验,其目的是在实验室里模拟检测商用CCD配备录像机后对星像的绝对及相对定位精度。通过使用不同图像板及录像带在不同幅度的CCD视频信号情况下的分组试验,得到了满足人卫观测的结果,CCD对绝对位置及相对位置的定位误差均小于±0.5个象元。本文还对误差产生的原因进行了初步分析。     

Spectral behaviour of the eclipsing binary TX UMa around primary minimum

Sixty-one blue spectrograms of TX UMa were obtained in the years 1969–1970, mainly in phases close to the primary minimum of the eclipsing system. The radial velocity curve displays clear rotational effect from which much higher than synchronous rotational velocity of the blue (B8V) component has been formally derived. However, this discrepancy is probably due to the presence of the tenous accretion disk around the primary. The disk is apparently fed by the intermittent mass transfer as indicated by the occasional changes of orbital period of the system. From all available radial velocity data an improved set of spectroscopic orbital elements is derived. The behaviour of the spectral lines in and out of the primary minimum is compared. Metallic lines of the cold (F7IV) secondary component are clearly seen exclusively in phases 0.988 to 0.012.Paper presented at the 11th European Regional Astronomical Meetings of the IAU on New Windows to the Universe, held 3–8 July, 1989, Tenerife, Canary Islands, Spain.     

有关内蒙古地质构造的一线之见——江苏响水至内蒙古满都拉地学断面北段研究报道之一

本文概述了江苏响水至内蒙古满都拉地学断面北段——包头至满都拉的地质观察结果。内容包括从太古宙乌拉山群到第四系、基底构造到新构造特征的七个方面。重点论述了渣尔泰群和白云鄂博群的构造性质,它们约在14亿年前才褶皱回返,代表了华北地台基底固结最迟的地段。造成这一事件的构造运动,拟称为色尔腾运动。此外,还讨论了华北地台北侧陆缘区加里东期和华力西期的构造     

The effects of climate change on heating energy consumption of office buildings in different climate zones in China

Theoretical and Applied Climatology - Climate plays an important role in heating energy consumption owing to the direct relationship between space heating and changes in meteorological conditions....