A complete relativistic ionized accretion disc in Cygnus X-1

The galactic black hole candidate Cygnus X-1 is observed to be in one of two X-ray spectral states: either the low/hard (low soft X-ray flux and a flat power-law tail) or high/soft (high blackbody-like soft X-ray flux and a steep power-law tail) state. The physical origin of these two states is unclear. We present here a model of an ionized accretion disc, the spectrum of which is blurred by relativistic effects, and fit it to the ASCA , Ginga and EXOSAT data of Cygnus X-1 in both spectral states. We confirm that relativistic blurring provides a much better fit to the low/hard state data and, contrary to some previous results, find the data of both states to be consistent with an ionized thin accretion disc with a reflected fraction of unity extending to the innermost stable circular orbit around the black hole. Our model is an alternative to those that, in the low/hard state, require the accretion disc to be truncated at a few tens of Schwarzschild radii, within which there is a Thomson-thin, hot accretion flow. We suggest a mechanism that may cause the changes in spectral state.     

Novel Analysis of Tadpole and Horseshoe Orbits

A simple analysis of tadpole and horseshoe orbits is performed using a new perturbation technique. The first-order results are presented explicitely, extension to any perturbation order is delineated. This revised version was published online in July 2006 with corrections to the Cover Date.     

The Hybrid Nature of 0846＋51W1： a BL Lac Object with a Narrow Line Seyfert 1 Nucleus

We found a NLS1 nucleus in the extensively studied eruptive BL Lac object, 0846+51W1, out of a large sample of NLS1s compiled from the spectroscopic dataset of SDSS DR1. Its optical spectrum can be well decomposed into three components: a power law component from the relativistic jet, a stellar component from the host galaxy, and a component from a typical NLS1 nucleus. The emission line properties of 0846+51W1, FWHM     

Evidence for Chemical Heterogeneity in the Nucleus of C/1995 O1 (Hale–Bopp)

We present an analysis of OH, CN, and C₂ jets observed in thecoma of Comet Hale–Bopp on UT April 22, 23, and 25, 1997. Monte Carlomodels designed to simulate the gas jets were employed to analyze thenuclear active areas responsible for the observed coma gas jets. Ourresults indicate that four active areas are necessary to reproduce theCN and C₂ jets while five active areas are required to simulatethe OH jets. The additional OH active area must produce significantlevels of OH, but cannot emit measurable quantities of either carbonradical. This difference suggests that the nucleus of Comet Hale–Boppis chemically heterogeneous.     

Comet Hale–Bopp: Velocity Field Of Ions From Fabry-Pérot Imaging

Fabry-Pérot interferograms of comet Hale-Bopp were obtained on several nights in March and April 1997. For this purpose we utilized the 2-channel focal reducer of the Max-Planck-Institute for Aeronomy at the 2-m telescope of the Pik Terskol Observatory. Solid Fabry-Pérot etalons of resolving power 30000 were used in both channels of the focal reducer. The main aim of this study is to measure the velocities and abundances of OH⁺ and H₂O⁺, both ions closely related to the same parent molecule, H₂O. In the blue channel interferograms we identified several individual OH⁺ rotational lines of the A³Π_i - X³Σ⁻ (0-0) transition and measured their Doppler shifts. The target emissions in the red channel were the H₂O⁺ lines of the A²A₁ − X²B₁ (10-0) band. We found that the line of sight velocities, obtained from the Doppler shifted wavelengths of emissions in the comet are higher in sunward direction than in the plasma tail and do not exceed 20 km s^–1. The corresponding values, deprojected in antisolar direction, are consistent with predictions by magnetohydrodynamical models of the solar-wind-comet interaction, when one accounts for the extremely high gas production rate of comet Hale-Bopp. This revised version was published online in July 2006 with corrections to the Cover Date.     

基于GIS技术的河流污染动态模拟系统

本文论述了稳态均匀流场中的一维河流水质扩散模型,并在此模型的基础上,基于GIS二次开发技术开发了河流污染动态模拟系统。该系统以乐山市涌斯江支流段的地理底图及基本数据为例,实现了对河流污染情况的动态模拟。通过对该系统的一系列操作,可以对河段任意位置污染物浓度进行自动查询和修改,从而为河流水质污染的监测和管理提供可视化参考依据。     

D-InSAR技术的积雪深度反演

积雪深度是大量气候、水文、农业及生态模型的重要输入变量。选用欧空局Sentinel-1主动微波数据,利用合成孔径雷达SAR(Synthetic Aperture Radar)差分干涉测量技术的二轨法,根据积雪相位与雪深之间的转换关系,反演新疆天山中段的巴音布鲁克盆地典型区的积雪雪深分布,提出了基于InSAR二轨差分的雪深估计方法,反演得到2016年12月18日的空间分辨率为13.89 m的雪深分布。研究表明:(1)对Sentinel-1数据进行正确的预处理以后,可以应用SAR差分干涉测量技术的二轨法反演区域雪深分布。但由于像对相干性和积雪状态的差异,积雪深度超过10 cm,可以获取较准确的雪深反演结果,R=0.65,反演误差的均方根误差RMSE=4.52 cm,平均相对误差为22.42%,反演雪深结果均比实测结果略偏低;而当雪深小于10 cm时,雪深反演值较实测值存在较大的误差,相对误差均高于34.52%,且反演雪深值均比实测值偏高。(2)雪深反演精度受高程及实际雪深的差异影响显著,另外雪深反演精度也受限于干涉像对相干性。结果表明,对于获取区域积雪雪深,InSAR技术较光学及被动微波遥感具有非常广阔的应用前景。     

Microscale Simultaneous Measurement of Carbon and Nitrogen Isotopes on Natural Diamond

Simultaneous analysis of carbon and nitrogen isotope ratios by SIMS was applied for the first-time to a natural diamond from the Kelsey Lake kimberlite, State Line Distinct, Colorado (UWD-1). This in situ procedure is faster, reduces sample size for analysis, and measures both isotope ratios from a single ~ 10 μm diameter pit, a critical advantage for zoned diamonds. The carbon isotope ratio (expressed as δ¹³C_VPDB) of the bulk UWD-1 crystal, determined by the conventional combustion method in the present study, is -5.9‰ ± 0.2‰ (VPDB, 2s). Nitrogen mass fraction ([N]) and isotope ratio (expressed as δ¹⁵N_Air) were determined by stepwise combustion and gas-source mass-spectrometry, resulting in 553 ± 64 μg g^-1 and -6.7‰ ± 1.1‰ (Air, 2s), respectively. Secondary ions of ¹²C₂^-, ¹²C¹³C^-, ¹²C¹⁴N^-, and ¹²C¹⁵N^- were simultaneously measured by SIMS using three Faraday cups and one electron multiplier. The spot-to-spot reproducibility of δ¹³C and δ¹⁵N values for the UWD-1 (178 spots on sixteen chips, 10 μm spots), were 0.3‰ and 1.6‰, respectively (2s). While ¹²C¹⁴N^-/¹²C₂^- ratios, which are an indicator for [N], varied up to 12% among these sixteen chips, such variation did not correlate with either δ¹³C or δ¹⁵N values. We propose that UWD-1 is a suitable reference sample for microscale in situ analysis of δ¹³C and δ¹⁵N values in diamond samples.     

银额盆地蒙苏地1井钻井设计与施工

蒙苏地1井是中国地质调查局部署在银额盆地艾特格勒凹陷的一口大口径重点油气地质调查井,根据该区块地层地质概况和钻井施工技术难点,从井身结构、钻具组合、钻头选型和钻进工艺等方面对蒙苏地1井钻井工程进行了优化设计。综合采用 “简化井身结构+非常规钻具组合+常规钻头选型+强抑制性泥浆”的钻井技术方案,解决了中生界巴音戈壁组和二叠系上部地层的高硬度、可钻性差、裂缝构造易井斜及井壁失稳等一系列难题,顺利完成了该井的钻井施工任务。该井完钻井深2763.66 m,完钻口径215.9 mm,平均机械钻速3.51 m/h,成功揭示了中生界和石炭-二叠系岩石组合特征及含油气性,优质、高效、零事故完成各项目标任务。