北京一号小卫星及其数据应用

结合小卫星技术介绍了北京一号高性能对地观测小卫星计划和项目进展情况,综述了北京一号系统的主要组成和性能,并结合其数据特点,介绍北京一号遥感影像的示范应用和重点应用,探讨、分析了其更广泛的应用领域和良好的市场前景。     

X-ray study of accretion flow in narrow-line Seyfert 1 galaxies

We present the results of a systematic study of narrow-line Seyfert 1 galaxies (NLS1s) observed with XMM-Newton. The 2–12 keV X-ray spectra of NLS1s are well represented by a single power law with a photon index Γ ∼ 2. When this hard power law continuum is extrapolated into the low energy band, we found that all objects in our sample show prominent soft excess emission. This excess emission is well parameterized by the thermal emission expected from an optically thick accretion disk, and we found the following three peculiar features: (1) The derived disk temperatures are significantly higher than the expectation from a standard Shakura-Sunyaev accretion disk, if we assume a central mass of a black hole to be 10^6–8M_⊙. (2) The temperatures are distributed within narrow range (ΔkT ∼ 0.08 keV) with an average temperature of 0.18 keV in spite of the range of four orders of magnitude in luminosity (10^41–45 erg s⁻¹). (3) We found a peculiar temperature–luminosity relation, where the luminosity seems to be almost saturated in spite of the significant change in temperature, during the observations of the most luminous NLS1 PKS 0558-504. These results strongly suggest that the standard accretion disk picture is no longer appropriate in the nuclei of NLS1s. We discuss a possible origin for the soft excess component, and suggest that a slim disk may be able to explain the observational results, if the photon trapping effect is properly taken into account.     

Cosmic background radiation from pregalactic objects

X-ray astronomy satellite TENMA observed that the X-ray pulsation of Vela X-1 suddenly disappeared for tens of minutes. This phenomenon may be interpreted in terms of the eclipse by a planet of HD77581, the optical companion of Vela X-1.     

浅析工业工程在质量QC小组活动中的运用

综述现代工业工程主要特点、基本工作方法及其在QC小组活动中的运用,提出了质量管理与工业工程有机结合,能够控制成本并使工作方法达到最优化。介绍了一个工业工程在QC小组活动中的运用实例。     

首都机场飞行流量的灰色区间预测

首都机场是中国航班最为密集的机场之一,科学准确地预测飞行流量的发展趋势,是首都机场各级决策部门制定发展规划的重要依据。区间预测相对于以往的单一值预测而言,能更好地反应出飞行流量的长期发展趋势,为辅助决策提供了一定的选择余地。针对飞行流量的长期预测存在影响因素较多、相关数据不足等特点,提出了以GM(1,N)模型为基础的灰色区间预测新模型,该模型利用指数回归模型得出的地区GDP的长期预测值,预测出年飞行流量未来的取值区间。通过对首都机场年飞行流量的仿真计算,说明该模型能够较好地显示出飞行流量的发展趋势。     

The iron Kα-line diagnostics of the rotating black hole metric in Seyfert galaxies

Observations of Seyfert galaxies in X-ray region reveal the wide emissive lines in their spectra, which can arise in inner parts of accretion disks, where the effects of General Relativity (GR) must be taken into account. A spectrum of a solitary emission line of a hot spot in Kerr accretion disk is simulated depending on the radial coordinate r and the angular momentum a = J/M of a black hole, under the assumption of equatorial circular motion of a hot spot. It is shown that the characteristic two-peak line profile with the sharp edges arises at a large distance (about r ≈ (3–10) r_g). The inner regions emit the line, which is observed with one maximum and extremely wide red wing. We present results of simulations for the isothermal and Shakura–Sunayev disks.     

Expectations for Crater Size and Photometric Evolution from the Deep Impact Collision

The NASA Discovery Deep Impact mission involves a unique experiment designed to excavate pristine materials from below the surface of comet. In July 2005, the Deep Impact (DI) spacecraft, will release a 360 kg probe that will collide with comet 9P/Tempel 1. This collision will excavate pristine materials from depth and produce a crater whose size and appearance will provide fundamental insights into the nature and physical properties of the upper 20 to 40 m. Laboratory impact experiments performed at the NASA Ames Vertical Gun Range at NASA Ames Research Center were designed to assess the range of possible outcomes for a wide range of target types and impact angles. Although all experiments were performed under terrestrial gravity, key scaling relations and processes allow first-order extrapolations to Tempel 1. If gravity-scaling relations apply (weakly bonded particulate near-surface), the DI impact could create a crater 70 m to 140 m in diameter, depending on the scaling relation applied. Smaller than expected craters can be attributed either to the effect of strength limiting crater growth or to collapse of an unstable (deep) transient crater as a result of very high porosity and compressibility. Larger then expected craters could indicate unusually low density (< 0.3 g cm⁻³) or backpressures from expanding vapor. Consequently, final crater size or depth may not uniquely establish the physical nature of the upper 20 m of the comet. But the observed ejecta curtain angles and crater morphology will help resolve this ambiguity. Moreover, the intensity and decay of the impact “flash” as observed from Earth, space probes, or the accompanying DI flyby instruments should provide critical data that will further resolve ambiguities.     

江苏省CBERS-1卫星红外数据应用示范研究评价

文章对CBERS -1卫星IRMSS数据从空间分辨率、几何精度、噪声等方面作了分析评价 ,选取典型的南京地区、洪泽湖作为示范应用区 ,经过几何精纠正后的IRMSS数据进行不同地物在不同波段上的光谱采样分析 ,进行了城市信息与湖泊信息提取实验 ,效果较好 ,对南京辖区和洪泽湖的形态特征、环境因素、动态变迁等方面作了分析研究 ,从图像上可以清晰地看出南京辖区水体、城建和交通以及郊区的农林状况、洪泽湖河口淤积、岸边污染的情况。总之 ,CBERS-1卫星IRMSS数据可用 ,质量较好 ,达到了设计要求 ,有广阔的应用前景。     

FY-1C/D极轨气象卫星空间粒子成分监测器及其在轨探测结果

介绍了风云一号(FY-1)C，D极轨气象卫星空间粒子成分监测器的任务目标、主要功能和工程指标。以及数据的获取和处理方法。给出了空间环境宁静期、地磁扰动事件、太阳质子事件、与太阳活动的关系和粒子长期变化等探测结果，并进行了相应的分析。对C，D星空间粒子成分监测器分别进行的5年和第二次在轨测试结果表明，两星监测器工作正常、性能稳定，探测数据可靠。     

CBERS-1红外遥感器图像处理系统设计

红外多光谱扫描仪（IRMSS）是中巴地球资源卫星（CBERS）上的重要有效载荷之一。其获取的红外图像可以在国民经济的各个领域得到广泛应用。但是由数传系统传回的图像数据不能直接用,必须经过相应的处理。文章介绍的内容就是如何设计一个处理系统,将这种不可直接用数据经过解码和图像格式的处理,得到可视图像;经过图像预处理,得到零级图像;经过相应的辐射校正处理,得到一级图像:经过几何校正处理,得到二级图像产品,提供给其它经济各部门加以应用。