64层CT回顾性心电门控低剂量冠脉成像的临床研究

目的：通过比较图像质量与辐射剂量,评价64层螺旋CT低剂量回顾性心电门控冠脉成像技术临床应用的可行性。方法：选取拟行CT冠状动脉造影的患者80例（心率小于65次/min,心率波动范围小于5次/min）,所选患者分为两组,分别进行低剂量回顾性心电门控（40例,开启ECG管电流调制技术,70%～80%期相满电流输出）及常规回顾性心电门控（40例,35%～80%期相满电流输出）CT冠脉造影,依据患者体质量指数选择管电流（400～800 mA）,管电压120 kV。比较两组的辐射剂量及图像质量。P〈0.05认为差异具有统计学意义。结果：低剂量回顾门控组与常规回顾门控组图像质量差异无统计学意义（Z=-4     

Full scale decay test of a tanker: field data and theoretical analysis

This paper presents results from a full scale decay test made with a tanker in a relatively protected area in the Brazilian coast. In at least two tests the environmental loads (wind, waves and current) were very small and the time history of the surge motion was well behaved, making it possible to check some proposed models for the damping in the hull and mooring lines. Field data seem to confirm that the damping is indeed of the fluid viscosity type and the theoretical models are able to recover roughly 75% of the observed damping, the energy dissipation in the mooring lines being, by far, the major contribution. The remaining 25% are likely due to non modeled effects, such as the environment influence, which although small and not measured certainly exists, and to the friction between the mooring lines and the seabed.     

地面气温观测系统设计与实验研究

为提高大气温度测量的准确度,本文设计了一种新型地面气温观测系统并推导了相应的辐射误差修正方程。首先,利用计算流体动力学（CFD）方法对该测温系统进行结构优化设计以及辐射误差量化计算。然后,利用BP神经网络算法拟合可针对多变量变化的辐射误差修正方程。最后,以076B型强制通风测温仪器的测量值作为温度基准,验证该测温系统的测温精度。实验结果表明,该新型地面气温观测系统的测量值与基准温度的均方根误差（RMSE）和绝对误差（MAE）分别为0.031 ℃和0.041 ℃。     

The unusual X-ray light curve of GRB 080307: the onset of the afterglow?

Swift -detected GRB 080307 showed an unusual smooth rise in its X-ray light curve around 100 s after the burst, at the start of which the emission briefly softened. This 'hump' has a longer duration than is normal for a flare at early times and does not demonstrate a typical flare profile. Using a two-component power-law-to-exponential model, the rising emission can be modelled as the onset of the afterglow, something which is very rarely seen in Swift -X-ray light curves. We cannot, however, rule out that the hump is a particularly slow early-time flare, or that it is caused by upscattered reverse shock electrons.     

Radiation–hydrodynamical collapse of pre-galactic clouds in the ultraviolet background

To explain the effects of the ultraviolet (UV) background radiation on the collapse of pre-galactic clouds, we implement a radiation–hydrodynamical calculation, combining one-dimensional spherical hydrodynamics with an accurate treatment of the radiative transfer of ionizing photons. Both absorption and scattering of UV photons are explicitly taken into account. It turns out that a gas cloud contracting within the dark matter potential does not settle into hydrostatic equilibrium, but undergoes run-away collapse even under the presence of the external UV field. The cloud centre is shown to become self-shielded against ionizing photons by radiative transfer effects before shrinking to the rotation barrier. Based on our simulation results, we further discuss the possibility of H₂ cooling and subsequent star formation in a run-away collapsing core. The present results are closely relevant to the survival of subgalactic Population III objects as well as to metal injection into intergalactic space.     

CONCENTRATION AND FLUX OF CO_2, TURBULENCE FLUXES AND RADIATION BALANCE IN THE NEAR SURFACE LAYER OVER WHEAT FIELD

The gradient of CO_2 concentration, photosynthetically active radiation (PAR). net radiation.soil heat flux, profiles of wind speed, and air temperature and humidity were measured above awheat field during May and June 1985 at Beijing Agro-Ecosystems Experimental Station. Beijing,China. Fluxes of carbon dioxide, sensible heat, latent heat and momentum were calculated byusing the aerodynamic method. The observation site. equipment, calibration techniques, theerrors associated with the measurement, and the computational procedures are described. Theresults show that the diurnal variations of amplitude of CO_2 concentrations were 103.8 to 27. 0. 86.3 to 22.8 and 69.8 to 11.6 ppm: the average CO_2 concentrations were 331.5. 339.9 and 364.6 ppmfor the photosynthesis type, and 369.6. 364.0 and 375.2 ppm for the respiration type at 1. 2 and10 m above surface, respectively, from May 14 to June 15. In the daytime, transfer direction ofthe CO_2 fluxes and gradients is from air to crop canopy, and at noon (1100 to 1300 BT (BeijingTime)) the transfer rate reaches negative maximum value. At night, transfer of CO_2 fluxes andgradients is in the reversed direction and reaches positive maximum in the early morning (0400 to0600 BT). There are strong negative correlations between CO_2 flux and the net radiation (Rn),available energy (H LE). photosynthetically active radiation (PAR) and momentum flux (τ).     

火星O2(a1Δg)气辉高光谱分辨辐射传输特性研究

1.27 μm波段的氧分子近红外气辉是火星大气最重要的气辉辐射之一, 该气辉高光谱分辨辐射传输模型的建立对于研制火星探测载荷, 反演火星大气的风场温度场与臭氧浓度, 以及研究火星空间物理, 有重要的科学价值与工程意义.在研究火星大气O₂(a¹Δ_g)气辉光化学反应模型的基础上, 提出了O₂(a¹Δ_g)气辉体辐射率的计算方法, 并建立了火星大气气辉辐射传输理论; 通过与用于研究火星大气特征的光谱学探测仪(Spectroscopy Spectrograph for the Investigation of Characteristics of the Atmosphere of Mars, SPICAM)的实测数据进行对比, 验证了所建立的火星O₂(a¹Δ_g)气辉高光谱分辨辐射传输模型的准确性; 针对火星与地球大气的O₂(a¹Δ_g)气辉, 在体辐射率、自吸收效应, 以及临边辐射光谱特性三个方面进行了系统深入的比较, 对比结果表明, 火星大气由于密度低、氧气丰度小, 其自吸收效应可以忽略不计, 但其O₂(a¹Δ_g)气辉辐射强度与地球大气相当, 可以用于火星大气的风场温度场与臭氧浓度的探测与反演.

     

青岛地区太阳紫外线辐射研究

通过对青岛地区2004年全年紫外线观测数据的分析,在预设局地纬度、海拔高度、大气中臭氧量及其分布、空气质量状况、地表反照率等因素基本不变的情况下,总结了青岛地区紫外辐射随与太阳天顶角相关的不同季节和时段、天气状况(云况)的统计性变化规律,以服务于该地区人们日常生活中对紫外线的防护,尤其是为调光生态膜的研制及改善提供参考。     

贵州青岩地区早-中三叠世生物地层

贵州青岩地区下-中三叠统发育齐全,化石丰富,尤其是中三叠世“青岩动物群”,具有生物辐射性质.为了研究二叠纪末生物大灭绝事件后的生物复苏及辐射过程,对该区下、中三叠统剖面进行了实测,并从沉积学、古生物学上进行了系统研究.识别出5个牙形石带:Neospathodus dieneri带、Neospathodus waageni带、Neospathodus pingdingshanensis带、Neospathodus homeri带、Chiosella timorensis带,建立2个有孔虫组合和6个双壳类组合.并根据牙形石化石初步确定出印度阶与奥伦尼克阶及奥伦尼克阶与安尼阶的界线.多门类化石的分布和生态组合结构表明,大灭绝后的复苏-辐射第一幕发生于安尼期早期,安尼期中期雷打坡页岩段的化石组合具有典型辐射后期的生态繁荣景象.古环境研究表明,本区从三叠纪初到中三叠世安尼期沉积水体总体上震荡式变浅,表现为盆地-陆棚-台缘斜坡-台地-盆地-台缘斜坡-陆棚的演变过程.