Mutual eclipses of J2 Europa by J1 Io observed at Yunnan Observatory in 2009

Mutual events between natural satellites include mutual occultation and mutual eclipse. Mutual eclipse is another kind of mutual occultation as viewed from the center of the Sun instead of the Earth. Two mutual eclipses of J2 Europa by J1 Io (2009 Aug. 28 and Sept. 12) were observed at Yunnan Observatory during the PHEMU09 international campaign. We will calculate the astrometric data of these Galilean satellites by analyzing and fitting the light curves we obtained. The limb-darkening was considered during...     

从永夏陈四楼煤矿水文地质特征看岩溶陷落柱并不存在

根据区域和矿区地质资料 ,结合岩溶陷落柱的形成地质条件进行认真的分析研究 ,得出了否定的认识 ,对正确认识永夏矿区的水文地质条件 ,有效地开展矿井防治水工作 ,正确指导生产有重要意义。     

基于OpenGL的GNSS仿真软件中的飞行模拟可视化研究

探讨利用OpenGL实现GNSS仿真软件中的飞行模拟可视化方法,给出根据仿真输出的俯仰角、偏航角和速度信息实现的三维可视化结果。     

Fiber Fine Structures Superposed on the Solar Continuum Emission Near 3 GHz

On April 21, 2002, a broadband solar radio burst was observed at about 01:00 – 03:00 UT with the digital spectrometers of National Astronomical Observatories of China (NAOC). Also many fiber bursts superposed on the continuum bursts were detected in the frequency range of 2.6 – 3.8 GHz during the time interval. After data processing, some parameters of the fibers such as frequency drift rate, duration, bandwidth, and relative bandwidth were determined. The mean value of the frequency drift was in the range of 42.3 – 87.4 MHz s⁻¹ (negative). A theoretical interpretation for the fibers was presented based upon a model of the velocity of Alfvén solitons. In this model, the source of the fiber emission was considered as the ducting of the solitons within the magnetic-mirror loop. Then the magnetic field strength of the fiber source was estimated to be about 130 ≤ B₀ ≤ 270 G. Also a comparison of the magnetic field estimation was made with another model of whistler group velocity.     

Solar Stokes Spectrum Observation at Yunnan Astronomical Observatory

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Excitation of Annual Polar Wobble by Global Oceans

A reasonable and quantitative result on the variation of polar wobble excited by the oceans is not available at present. Numerous researches have shown that atmospheric motion is the greatest excitation source for the seasonal variations in the polar wobble and that oceanic motion is one of the main remaining excitation sources. The excitation of variation in the annual polar wobble caused by oceans from 1992 to 2004 both globally and in latitude dependence, have been studied in depth by means of the new generation of SODA oceanic data assimilation (SODA-1.4.2 and SODA-1.4.3) and the ECCO oceanic data assimilation. The result shows that the variation in the seasonal polar wobble excited by the SODA oceans is very close to that of the residual after the action of the atmosphere and land water is deducted from the geodesic excitation function for a large part of the investigated time interval, and that there is overall agreement between the two as regards the annual amplitude and phase. In addition, in comparison with the result of early SODA-Bata 7, the new generation of SODA oceanic excitation has achieved obvious improvements. The latitude distributions of the excitations of the annual polar wobble by the SODA and ECCO oceans are consistent in the Greenwich direction, while having obvious differences in the direction of 90° E.     

AMR Simulations of Magnetohydrodynamic Problems by the CESE Method in Curvilinear Coordinates

The objective of this paper is to present new extensions of the space – time conservation element and solution element (CESE) method for simulations of magnetohydrodynamic (MHD) problems in general curvilinear coordinates by using an adaptive mesh refinement (AMR) grid system. By transforming the governing MHD equations from the physical space (x,y,z) to the computational space (ξ,η,ζ) while retaining the form of conservation, the CESE method is established for MHD in the curvilinear coordinates. Utilizing the parallel AMR package PARAMESH, we present the first implementation of applying the AMR CESE method for MHD (AMR-CESE-MHD) in both Cartesian and curvilinear coordinates. To show the validity and capabilities of the AMR-CESE-MHD code, a suite of numerical tests in two and three dimensions including ideal MHD and resistive MHD are carried out, with two of them in both Cartesian and curvilinear coordinates. Numerical tests show that our results are highly consistent with those obtained previously by other authors, and the results under both coordinate systems confirm each other very well.     

邵东保和堂大冶灰岩沉积构造特征

保和堂大冶灰岩中发育丰富的沉积构造,对之研究有助于保和堂、乃至整个湘中的大冶灰岩形成环境的探讨。其第一段岩石发育了丘状波痕、丘状交错层理及粒序层理,是风暴作用的反映;泥裂、水雹痕属于暴露环境。说明大冶灰岩沉积的早期仍属潮上或潮间碳酸盐台地相。中期海水加深,发育了水平层理、变形层理及包卷层理等,近于台地边缘斜坡相。晚期的粒序层理、虫迹等构造,反映了海水再度变浅的趋势。     

青藏铁路清水河地区路基下伏多年冻土地温变化特征研究

基于埋设在青藏铁路清水河地区路基中两个断面内的共8个地温测试孔3年来的地温观测资料,研究了该地区铁路路基下伏高原多年冻土融化特征,分析了多年冻土上限的变化规律以及填筑铁路路基施工对下伏多年冻土赋存条件的影响。研究表明,由于受到填筑路基时赋存在路基填料内的热量的影响,铁路路基下伏多年冻土近地表的地温变化特征与天然地面下的多年冻土的地温变化特征有明显的不同,且向阳面与被阴面差别较大。多年冻土的上限在施工初期会有一个明显的下移沉降,随着时间的推移,虽然残存在路基中的热量逐渐消散,多年冻土上限下降会逐渐稳定。由于受到太阳辐射和路基边坡形状及融化夹层的影响,多年冻土上限会逐渐稳定,但不会在短时期内上升到天然地面下多年冻土的上限水平。     

滇西北铜厂沟Mo-Cu矿床岩体年代学、地球化学及其地质意义

铜厂沟大型斑岩型Mo-Cu多金属矿床位于扬子西缘义敦岛弧带南端,钼矿化与花岗闪长斑岩紧密相关。花岗闪长斑岩LA-ICP-MS锆石U-Pb年龄为84.57±0.29Ma(MSWD=0.73),侵位于晚白垩世。岩石的Si O2为63.03%~69.60%,Na2O+K2O为6.97%~9.11%,具高钾钙碱性和准铝质-弱过铝质(A/CNK=0.88~1.05)特征。岩石富集轻稀土元素和大离子亲石元素(Rb、Ba、Pb等),相对亏损重稀土元素和高场强元素(Ti、Nb、P等),并且具有较高的Sr/Y和La/Yb比值,及较低的Y、Yb及Mg O含量。这些地球化学特征表明铜厂沟花岗闪长斑岩具有埃达克质岩石的特征,可能起源于加厚下地壳岩石的部分重熔。地球化学投图显示,铜厂沟岩体呈现出晚碰撞-碰撞后花岗岩特征,指示着岩体可能形成于陆内碰撞造山后由挤压转换为伸展构造环境;岩浆上侵过程中含矿热液沿构造发育部位运移,在酸性岩体内形成细脉浸染状钼(铜钨)矿化,在构造破碎带、层间滑动带和玄武岩与碳酸盐岩接触带交代形成矽卡岩型Cu、Pb、Zn多金属矿体和热液脉型Pb、Zn、Ag多金属矿体,构成钼(铜钨)→铜钼→铁铜金→铅锌的成矿元素分带和斑岩成矿系统。