太阳耀斑的厘米波和分米波射电辐射

综述了太阳厘米波射电源的形态特征和演化，以及厘米波辐射与X射线源的特性比较；介绍了太阳分米波射电辐射的一些最观测结果，包括分米波Ⅲ型爆发、纤维结构、斑马纹结构、DPS漂移脉动结构、spike尖峰辐射等多种精细结构，并讨论了可能的辐射机制。     

Active Galaxies in the UV

In this article we present different aspects of AGN studies demonstrating the importance of the UV spectral range. Most important diagnostic lines for studying the general physical conditions as well as the metalicities in the central broad line region in AGN are emitted in the UV. The UV/FUV continuum in AGN excites not only the emission lines in the immediate surrounding but it is responsible for the ionization of the intergalactic medium in the early stages of the universe. Variability studies of the emission line profiles of AGN in the UV give us information on the structure and kinematics of the immediate surrounding of the central supermassive black hole as well as on its mass itself.     

A high galactic latitude HI 21 cm-line absorption survey using the GMRT: II. Results and interpretation

We have carried out a sensitive high-latitude (|b| > 15°) HI 21 cm-line absorption survey towards 102 sources using the GMRT. With a 3σ detection limit in optical depth of ∼ 0.01, this is the most sensitive HI absorption survey. We detected 126 absorption features most of which also have corresponding HI emission features in the Leiden Dwingeloo Survey of Galactic neutral Hydrogen. The histogram of random velocities of the absorption features is well-fit by two Gaussians centered at V_1sr ∼ 0 km s⁻¹ with velocity dispersions of 7.6 ± 0.3 km s⁻¹ and 21 ± 4 km s⁻¹ respectively. About 20% of the HI absorption features form the larger velocity dispersion component. The HI absorption features forming the narrow Gaussian have a mean optical depth of 0.20 ± 0.19, a mean HI column density of (1.46 ± 1.03) × 10²⁰ cm⁻², and a mean spin temperature of 121 ± 69 K. These HI concentrations can be identified with the standard HI clouds in the cold neutral medium of the Galaxy. The HI absorption features forming the wider Gaussian have a mean optical depth of 0.04 ± 0.02, a mean HI column density of (4.3 ± 3.4) × 10¹⁹ cm⁻², and a mean spin temperature of 125 ± 82 K. The HI column densities of these fast clouds decrease with their increasing random velocities. These fast clouds can be identified with a population of clouds detected so far only in optical absorption and in HI emission lines with a similar velocity dispersion. This population of fast clouds is likely to be in the lower Galactic Halo.     

基于重构等高线的格网细化模型

以规则格网DEM为基础,利用回放等高线与原等高线进行比较,提出两个误差指标和一种格网细化模型,以生成多分辨率的格网DEM,并提高DEM的等高线精度。针对该模型的两个关键步骤,进行了较为详细的论述。通过对一幅实际地形数据进行试验,比较不同方法得出的DEM等高线精度,为DEM精度研究,特别是多分辨率DEM精度研究,提供了一种新的方法和思路。     

Thermo-economic Investigation of an Enhanced Geothermal System Organic Rankine Cycle and Combined Heating and Power System

As a potentially viable renewable energy, Enhanced Geothermal Systems (EGSs) extract heat from hot dry rock (HDR) reservoirs to produce electricity and heat, which promotes the progress towards carbon peaking and carbon neutralization. The main challenge for EGSs is to reduce the investment cost. In the present study, thermo-economic investigations of EGS projects are conducted. The effects of geofluid mass flow rate, wellhead temperature and loss rate on the thermo-economic performance of the EGS organic Rankine cycle (ORC) are studied. A performance comparison between EGS-ORC and the EGS combined heating and power system (CHP) is presented. Considering the CO2 emission reduction benefits, the influence of carbon emission trading price on the levelized cost of energy (LCOE) is also presented. It is indicated that the geofluid mass flow rate is a critical parameter in dictating the success of a project. Under the assumed typical working conditions, the LCOE of EGS-ORC and EGS-CHP systems are 24.72 and 16.1 cents/kWh, respectively. Compared with the EGS-ORC system, the LCOE of the EGS-CHP system is reduced by 35%. EGS-CHP systems have the potential to be economically viable in the future. With carbon emission trading prices of 12.76 USD/ton, the LCOE can be reduced by approximately 8.5%.     

粉末压片制样-X射线荧光光谱法分析地球化学调查样品测量条件的优化

在X射线荧光光谱(XRF)分析中,粉末压片制样是被广泛应用的一种制样方法,但由于存在样品粒度、矿物和基体效应对其测量条件进行优化。本文应用XRF法测量地球化学调查样品中24种主次量元素,综合优化了制样压力、仪器工作电压和工作电流、待测元素分析谱线、探测器的调节和探测效率等实验条件。在最优测量条件下,用土壤和水系沉积物国家标准物质GBW07402、GBW07404、GBW07424、GBW07426、GBW07429验证方法的准确度,结果表明个别元素如GBW07402中的Na2O、GBW07404中的Pb相对误差大于10%,其余元素的相对误差小于10%,但均达到了地球化学调查样品的质量监控要求。经优化的仪器测量条件为我国地球化学调查样品提供了可靠的基础数据。