海尔—波普彗星的CO（J=1—0）谱线的观测

使用紫金山天文台青海观测站13．7米毫米波射电望远镜,于1996年12月10日至1997年1月2日和1997年3月25日至1997年4月4日对海尔－波普彗星的CO分子J＝1—0转动跃迁谱线（频率为115．27120GHz）进行了观测．观测谱线表明,CO分子相对于地心的速度比彗星整体相对于地心的速度要小些,即有蓝移现象．这反映了CO分子是由该彗星迎着太阳的面以一定的速度产生出来的．从观测谱线中还初步估算了该彗星CO分子的产生速率．     

Precise Synchrotron Radiation Spectrum of Fast-cooling Electrons and the Prompt GRB Emission

It is generally believed that the synchrotron radiation of electrons from the internal shock is the main radiation mechanism of the prompt GRB (gamma-ray burst) emission. However, what this model predicts can not explain observations well. In this paper, we confirm that electrons are quickly cooled due to radiation losses and also point out that the synchrotron radiation spectrum presented in previous papers is a relatively rough estimation. We get the precise synchrotron radiation spectrum of fast-cooling electrons by carrying out a numerical calculation, and thereby reasonably explain the observed distribution of low-energy spectral index (α) of long GRBs based on a unified model. In addition, we fit the correlation between α and the peak energy of the νFν spectrum (E_p).     

Star forming activities in W75N and DR21 – Are the two regions in collision?

We have observed the massive star formation region W75N in ¹²CO J = 3 ? 2 with KOSMA. The profile of ¹²CO J = 3 ? 2 indicated that besides the 9 km s^?1 component, there is another component of ?3 km s^?1, which is associated with another star formation region, DR21N, located to the north of DR21. We derived the physical and dynamical parameters of the core and high velocity gas associated with the two components separately. Star forming activities were investigated, including outflows and infall analysis. The two regions overlap in space and are not connected in velocity. We found that the cloud–cloud collision scenario may not apply for the DR21/W75N case.     

云南天文台基本天体测量工作的发展

介绍了云南天文台天体测量工作的发展过程，论述了在空间时代地面光学基本天体测量的必要性和应具备的条件，并且叙述了在新的要求和条件下，地面光学基本天体测量工作应该发挥的作用和广阔的发展前景。     

Last glacial terrestrial vegetation record of leaf wax n-alkanols in the northern South China Sea: Contrast to scenarios from long-chain n-alkanes

Long-chain n-alkanols and n-alkanes in core sediments from the northern South China Sea (SCS) were measured to make a comparison during terrestrial vegetation reconstruction from ~42 ka to ~7 ka. The results showed that terrestrial vegetation record from long-chain n-alkanes matched well with previous studies in nearby cores, showing that more C₄ plants developed during the Last Glacial Maximum (LGM) and C₃ plants dominated in the interglacial period. However, these scenarios were not revealed by terrestrial vegetation reconstruction using long-chain n-alkanols, which showed C₃ plant expansion during the LGM. The discrepancy during the interglacial period could be attributed to the aerobic degradation of functionalized long-chain n-alkanols in the oxygen-rich bottom water, resulting in poor preservation of terrestrial vegetation signals. On the other hand, the different advantages of functionalized n-alkanols and non-functional n-alkanes to record local and distal vegetation signals, respectively, may offer a potential explanation for the contradiction during the LGM when the SCS was characterized by low-oxygen deep water. Nevertheless, large variations on n-alkyl lipid compositions in C₃/C₄ plants could play a part in modulating sedimentary long-chain n-alkanols and n-alkanes toward different vegetation signals, thereby suggesting that caution must be taken in respect to the terrestrial vegetation reconstruction using long-chain n-alkanes and long-chain n-alkanols.     

基于AMT的龙首山成矿带西岔地段马路沟断裂带深部发育特征

为减少铀矿钻探工程风险,基于音频大地电磁法(AMT)资料,对龙首山成矿带中的马路沟断裂及次级断裂的深部发育特征进行了探究。通过对马路沟断裂与次级断裂正演理论模型响应特征分析,论证了方法的可行性,在此基础上,结合地质、岩石电性参数和钻探资料,对反演电阻率断面进行了推断解释,大致查明了区内断裂的深部发育特征。研究结果表明:马路沟断裂(F101)走向NW,倾角约80°,其中X501—X502剖面之间倾向NE,X502—X506剖面倾向SW;次级断裂F102、F103走向NW,均倾向NE,倾角75°~80°;上述断裂具有切割深度大、倾角较陡特征。该结果为后期钻探工程的布置提供了依据,提升了铀矿地质勘查的效果与效益。     

沧县隆起北部地区地热资源特征及开发潜力

【研究目的】地热资源特征研究及开发潜力分析是开发区域地热资源的重要依据。【研究方法】本文将前人研究成果与最新钻井资料相结合,通过对沧县隆起北部地区地热地质背景、热储分布、地温场特征、水化学资源类型等主要因素进行剖析,建立了该区的地热成藏模式。【研究结果】沧县隆起北部地区是在渤海湾伸展型沉积盆地高大地热流值背景下,由北部燕山裸露区基岩接受的大气降水作为近源补给水源,进入基岩的冷水在深层循环过程中受到深部热源加热增温,沿断裂破碎带和不整合面向上运移富集,形成的以传导型传热机制为主的地热系统。【结论】本区地热资源特点为热储类型多、盖层地温梯度高、补给速度快、资源量巨大。主要表现为：区内分布馆陶组砂岩热储,奥陶系、蓟县系雾迷山组岩溶热储三套主力热水储集层;地温场分布主要受基底构造形态控制,基岩凸起区的平均地温梯度为45℃/km;地下水类型随着埋深的增加由HCO₃-Na、HCO₃·SO₄-Na型水向成熟的Cl-Na型水过渡;本区内三套热储的可采地热资源量为1.67×10¹⁰GJ,折合标煤5.72×10⁸t,年可开采地热资源量可满足供暖面积2亿m²,若在采灌平衡的条件下,沧县隆起北部地区年可采地热资源量为7.06×10⁷GJ,折合标煤2.41×10⁶t,可满足供暖面积0.85亿m²,具有良好的地热市场开发前景。     

天然气中甲烷和CO2的二元同位素特征

不同成因的天然气由于形成温度不同,往往会有不同的稳定同位素特征。但是,由于经常不能同时获得天然气以及它的生成母体的同位素成分,很难用单独的C或H同位素成分来确定它的形成温度。在形成天然气时,不同的温度会形成不同的二元同位素的浓度,温度越低,二元同位素的比例越大,因此只需要知道天然气本身的二元同位素的浓度,就可以确定形成温度,从而避免了需要知道天然气生成母体的同位素成分这一难题。本文利用高级量子化学计算,预测了不同温度下天然气中甲烷和CO2气体的二元同位索（Clumped isotope）的特征,提供用于天然气成因分析的新方法。     

Rhuddanian to Aeronian (Llandovery,early Silurian) carbon isotope stratigraphy throughout carbonate sequences in the upper Yangtze region,South China block

The Xiangshuyuan Formation (middle Rhuddanian to middle Aeronian stages of the Llandovery Series, lower Silurian) records a shelly fauna representing recovery after the end-Ordovician mass extinction in a well-oxygenated shallow carbonate platform of the Upper Yangtze region, South China Block. Carbon isotope stratigraphy is documented from limestone sequences of the formation at the Qiankou section, northeast Guizhou. The early Aeronian carbon isotope excursion (EACIE, with an amplitude of about 2 ‰ and peak value of 2.44 ‰) is identified in the middle and upper parts of the formation (Ozarkodina obesa conodont Biozone). The EACIE recorded herein correlates well with those in Baltica, Canada, and the United States; together with its records from organic material (δ¹³C_org) the data verify that the EACIE is a global event. The beginning of the EACIE can be used as a chemostratigraphic marker defining the Rhuddanian/Aeronian boundary in strata that lack high-resolution biostratigraphic constraints.