天然气水合物和游离气饱和度估算的影响因素

讨论了不同水合物胶结类型的流体饱和多孔隙固体中地震波的衰减情况,分析了估算天然气水合物和游离气饱和度影响因素.结果表明, 地层孔隙度、纵波速度模型和弹性模量的计算方法是影响反演水合物和游离气饱和度的关键因素.含水合物地层的吸收与水合物胶结类型密切相关,当水合物远离固体颗粒,像流体一样充填在孔隙时,品质因子出现负异常,而当水合物胶结固体颗粒影响骨架的弹性性质,其品质因子出现正异常.根据布莱克海台地区164航次995井的测井资料,分别应用低频和高频速度模型估算了水合物和游离气饱和度.由低频速度模型得到的水合物饱和度(占孔隙空间的)10%～20%,游离气饱和度(占孔隙空间的)0.5%～1%;而由高频速度模型得到的水合物饱和度(占孔隙空间的)5%～10%,游离气饱和度(占孔隙空间的)1%～2%.     

地应变震兆异常信息提取方法研究

分析了怀来台体积应变观测资料的特点,研究了体积应变观测资料的气压干扰、仪器漂移的剔除方法和预处理后的资料分析方法,在分析中发现,振幅因子和非潮汐应变速率在1996年以来,在首都圈地区中西部发生的中强地震前,均有大小不同、持续时间不等的异常,这些参数可作为怀来地震台今后地震分析和地震中短期预测的指标。     

干旱区土地荒漠化中人类因素分析

目前干旱区突出的矛盾是,人类活动对环境的负效应在总体上已导致以土地荒漠化急剧发展为主的生态环境质量显著下降。基于1994年“联合国防治荒漠化公约”给出的土地荒漠化概念和干旱区的特点,划分土地荒漠化的自然因素和人为因素。通过人类活动的涵义和特点的探讨,首次全面和综合地分析了土地荒漠化发展中的人类活动因素,包括人类活动的驱动作用、人类各种活动方式的作用和人类活动的管理作用等。依据一定的原则,构建出适用于干旱区人类活动对土地荒漠化作用的指标体系,该指标体系多为量化指标并可反映人类活动的动态变化,可为人类活动在土地荒漠化中作用的更进一步(定量)研究提供依据。     

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Kinematics and stellar populations of the dwarf elliptical galaxy IC 3653

We present the first 3D observations of a diffuse elliptical galaxy (dE). The good quality data (S/N up to 40) reveal the kinematical signature of an embedded stellar disc, reminiscent of what is commonly observed in elliptical galaxies, though similarity of their origins is questionable. Colour map built from Hubble Space Telescope Advanced Camera for Surveys (ACS) images confirms the presence of this disc. Its characteristic scale (about 3 arcsec =250 pc) is about a half of galaxy's effective radius, and its metallicity is 0.1–0.2 dex larger than the underlying population. Fitting the spectra with synthetic single stellar populations (SSP), we found an SSP-equivalent age of 5 Gyr and nearly solar metallicity [Fe/H]  =−0.06  dex. We checked that these determinations are consistent with those based on Lick indices, but have smaller error bars. The kinematical discovery of a stellar disc in dE gives additional support to an evolutionary link from dwarf irregular galaxies due to stripping of the gas against the intracluster medium.     

Five WC9 stars discovered in the AAO/UKST Hα survey

We report the discovery of five massive Wolf–Rayet (WR) stars resulting from a programme of follow-up spectroscopy of candidate emission-line stars in the Anglo-Australian Observatory United Kingdom Schmidt Telescope (AAO/UKST) Southern Galactic Plane Hα survey. The 6195–6775 Å spectra of the stars are presented and discussed. A WC9 class is assigned to all five stars through comparison of their spectra with those of known late-type WC stars, bringing the known total number of Galactic WC9 stars to 44. Whilst three of the five WC9 stars exhibit near-infrared (NIR) excesses characteristic of hot dust emission (as seen in the great majority of known WC9 stars), we find that two of the stars show no discernible evidence of such excesses. This increases the number of known WC9 stars without NIR excesses to seven. Reddenings and distances for all five stars are estimated.     

冬季影响北疆高速公路行车安全的气象要素特征分析

利用1961—2007年长达47a高速、高等级公路沿线气象站的资料,重点研究北疆高速、高等级公路沿线冬季影响车辆安全行驶的气象要素的气候特征,分析该路段降雪、积雪、结冰、冻雨等气象要素的时间和空间分布,并依据气候分布特点从气候的角度将北疆高速、高等级公路沿线路段按降雪、积雪、结冰、冻雨等对行车安全影响程度划分为极易打滑路段、较易打滑路段、易打滑路段和不易打滑路段,为公路管理部门提供科学的、合理的防御和减少冬季交通事故的理论依据。     

On the Red Rectangle optical emission bands

We have observed the Red Rectangle nebula with the Multi-Object Spectrograph on the WIYN telescope. Moderate-resolution spectra (Δ λ =0.4 Å) in the region of 5800 Å were obtained in 3-arcsec apertures at over 50 positions in the nebula. Accurate and precise wavelength calibrations were obtained against a thorium–argon lamp and the sodium lines in the sky and nebula. The peak position and full width at half-maximum of the 5800-Å Red Rectangle band (RRB) were measured to beyond 15 arcsec from the star. The shortest wavelength of the band is found to be 5799.10±0.15 Å in the rest frame of the nebula. None of the emission bands has intensity coincident with the wavelength of the diffuse interstellar band (DIB) at 5797.11±0.05 Å. The 2-Å offset cannot be explained by an instrumental, spectroscopic or photophysical effect. The hypothesis that the same molecule may be the carrier of the RRB and the DIB is contradicted by these observations. As a further test of the hypothesis, absorption has been sought that would be due to a potential DIB carrier in the nebula. Tentative evidence for absorption is found in the RRB spectra taken within 9 arcsec of the star; but any absorption has a peak position essentially coincident in wavelength with the band maximum of the emission band.     

用日全食光谱探测太阳中低层大气对局部热动平衡的偏离

在太阳大气不同层次连续光谱中叠加有丰富的发射线或吸收线,对这些谱线轮廓进行反演分析可以探测太阳大气的化学成分和物理状态.太阳大气的色球及过渡区由于其密度低难以建立热动平衡,建立相应的大气模型需要采用非局部热动平衡(Non-Local Thermodynamic Equilibrium,N-LTE)理论.根据相对偏离因子计算来研究太阳中低层大气偏离局部热动平衡(Local Thermodynamic Equilibrium,LTE)分布的情况.首先对日全食观测过程中得到色球和过渡区不同高度形成的两条光谱数据进行反演,得到确定观测谱线的参数信息,如连续谱源函数、谱线源函数、多普勒宽度和由此推出的等效动力学温度;根据这些反演出的谱线参量计算出二维视场内每个空间采样点偏离LTE状态的定量结果;其次,根据用于观测的积分视场单元光纤排布阵列重构出辐射强度、等效动力学温度和相对偏离因子二维分布.结果显示:在局部小区域,温度分布和相对偏离因子的分布存在较强相关性,而与辐射强度分布无明显相关.从两条谱线导出的等效温度和相对偏离因子分布存在明显的差异.这两种二维分布揭示出太阳大气某些小尺度区域具有较强的结构性和复杂性,为进一步理解太阳中低层大气物理提供了一种新的视角.