Approaches and countermeasures of the transfer of rural surplus labors in China

IntroductionThe trallSfer of ~l sUrplus labor is a great and occult socio-economic project ti'ans-centUry in Chin4which is closely related to the development of agricultUre and the whole national economy. To someextent it decides the ~nnation from the System of tWo layers to modendsahon in economy and thedevelopment from laggard agriculed counny tO rising industrialized one as well as makes the edeconomy go up to the new Stage so as to achieve the compalatively well-off goal. ESPecially on…     

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.     

Massive star formation in galaxies: radiative transfer models of the UV to millimetre emission of starburst galaxies

We present illustrative models for the UV to millimetre emission of starburst galaxies which are treated as an ensemble of optically thick giant molecular clouds (GMCs) centrally illuminated by recently formed stars. The models follow the evolution of the GMCs owing to the ionization-induced expansion of the H  ii regions and the evolution of the stellar population within the GMC according to the Bruzual & Charlot stellar population synthesis models. The effect of transiently heated dust grains/PAHs on the radiative transfer, as well as multiple scattering, is taken into account.
The expansion of the H  ii regions and the formation of a narrow neutral shell naturally explain why the emission from PAHs dominates over that from hot dust in the near- to mid-infrared, an emerging characteristic of the infrared spectra of starburst galaxies.
The models allow us to relate the observed properties of a galaxy to its age and star formation history. We find that exponentially decaying 10⁷–10⁸ yr old bursts can explain the IRAS colours of starburst galaxies. The models are also shown to account satisfactorily for the multiwavelength data on the prototypical starburst galaxy M82 and NGC 6090, a starburst galaxy recently observed by ISO . In M82 we find evidence for two bursts separated by 10⁷ yr. In NGC 6090 we find that at least part of the far-infrared excess may be due to the age of the burst (6.4×10⁷ yr). We also make predictions about the evolution of the luminosity of starbursts at different wavelengths which indicate that far-infrared surveys may preferentially detect older starbursts than mid-infrared surveys.     

Ionizing radiation in smoothed particle hydrodynamics

A new method for the inclusion of ionizing radiation from uniform radiation fields into 3D smoothed particle hydrodynamics (SPHI) simulations is presented. We calculate the optical depth for the Lyman continuum radiation from the source towards the SPHI particles by ray-tracing integration. The time-dependent ionization rate equation is then solved locally for the particles within the ionizing radiation field. Using test calculations, we explore the numerical behaviour of the code with respect to the implementation of the time-dependent ionization rate equation. We also test the coupling of the heating caused by the ionization to the hydrodynamical part of the SPHI code.     

Optical properties of the carbon dust grains in the envelopes around asymptotic giant branch stars

We have investigated the optical properties of the carbon dust grains in the envelopes around carbon-rich asymptotic giant branch stars, paying close attention to the infrared observations of the stars and the laboratory-measured optical data of the candidate dust grain materials. We have compared the radiative transfer model results with the observed spectral energy distributions of the stars including IRAS Point Source Catalog and IRAS Low Resolution Spectrograph data. We have deduced an opacity function of amorphous carbon dust grains from model fitting with infrared carbon stars. From the opacity function, we have derived the optical constants of the AMC grains. The optical constants satisfy the Kramers–Kronig relation and produce the opacity function that fits the observations of infrared carbon stars better than previous works in the wide wavelength range 1–1000 μm. We have used simple mixtures of the AMC and silicon carbide grains for modelling. We have compared the contributions that AMC and SiC grains make to the opacity for the cases of simple mixtures of them and spherical core–mantle type grains consisting of a SiC core and an AMC mantle .     

地面GPS探测大气的最新进展

综述了利用地面ＧＰＳ站探测大气的技术，包括基本原理，方法，应用，最新进展和结果的介绍以及存在于该技术的误差源的讨论。从地面ＧＰＳ站的观测和表面气象参数可得出天顶湿延迟的估计，再由它和可降水汽量之间的转换关系就可得出ＰＷＶ估计。这种方法求得的ＰＷＶ时间序列不仅能提高天气预报的准确度而且有助于气候变化的研究和数值天气预报模型的改进，这就是新兴学科ＧＰＳ气象学形成的基础。     

波纹开缝翅片管换热器传热与流动性的数值模拟

提出一种波纹开缝翅片管换热器,对其传热与流动特性进行三维数值模拟,选择Re范围在1 000到5 000时与平板开缝翅片的模拟相比较。结果表明,在Re小于2 752时,平板开缝比波纹开缝的换热效果好,而Re大于2 752时,波纹开缝比平板开缝换热效果更好,并且波纹开缝翅片管换热器的流动阻力小于平板开缝,因此,Re大于2 752时波纹开缝比平板开缝综合效果更好。     

中国沿海HY-2A校正微波辐射计水汽含量数据精度检验方法

为评价“海洋二号”卫星（HaiYang-2A, HY-2A）校正微波辐射计（Calibration Microwave Radiometer, CMR）近海水汽产品精度,以中国沿海全球导航卫星系统（Global Navigation Satellite System, GNSS）业务观测站数据和欧洲中期天气预报中心（European Centre for Medium-Range Weather Forecasts, ECMWF)发布的第五代大气再分析资料（ECMWF Reanalysis 5, ERA5）作为验证数据。首先对选取的GNSS业务观测站数据和CMR水汽含量数据进行时空匹配,两者的观测时间一致、空间范围取为100 km;然后利用精密单点定位方法反演GNSS业务观测站上空的大气可降水量（Precipitable Water Vapor, PWV）,同时对1 h分辨率的ERA5再分析资料内插计算,得到CMR水汽数据点处的ERA5 PWV;最后以GNSS PWV和ERA5 PWV为参考,分析2015年CMR水汽产品精度和偏差时空分布。结果表明,CMR水汽含量和GNSS PWV、E...     

Transnational technology transfer network in China: Spatial dynamics and its determinants

Patent transfer has been regarded as an important channel for the nations and regions to acquire external technology, and also a direct research object to depict the relationship between supply and demand of technology flow. Therefore, based on traceable patent transfer data, this article has established a dual-pipeline theoretical framework of transnational-domestic technology transfer from the interaction of the global and local(glocal)perspective, and combines social networks, GIS spatial ana...