2018年湖南省农村自然灾害社会脆弱性测度

农村社会发展状况与自然灾害发生频率和强度息息相关,提高农村自然灾害社会脆弱性对农村社会发展及实现乡村振兴战略具有重要作用。以湖南省各地级市州农村为研究对象,从敏感性和恢复力两个维度建立社会脆弱性指标评价体系,采用熵值法、模糊综合评价法和函数法测算敏感性、恢复力和脆弱性指数,分析2018年湖南省农村自然灾害社会脆弱性。结果表明,湖南省农村社会脆弱性空间分异特征明显,呈现“东低西高”的分布格局;多数地区的农村社会脆弱性处于低位水平,地区分异显著,具有两极分化分布特点,张家界地区最高,长沙和衡阳地区最低。在中低社会脆弱性的农村,恢复力指数对社会脆弱性贡献最大,其中最为显著的便是社会公共事业的建设水平和基础设施的完善水平。在高社会脆弱性的农村,敏感性指数对社会脆弱性贡献度最大。     

Data processing and initial results from the CE-3 Extreme Ultraviolet Camera

The Extreme Ultraviolet Camera(EUVC) onboard the Chang'e-3(CE-3)lander is used to observe the structure and dynamics of Earth's plasmasphere from the Moon. By detecting the resonance line emission of helium ions(He+) at 30.4 nm, the EUVC images the entire plasmasphere with a time resolution of 10 min and a spatial resolution of about 0.1 Earth radius(RE) in a single frame. We first present details about the data processing from EUVC and the data acquisition in the commissioning phase, and then report some initial results, which reflect the basic features of the plasmasphere well. The photon count and emission intensity of EUVC are consistent with previous observations and models, which indicate that the EUVC works normally and can provide high quality data for future studies.     

基于时间序列法的北京市需水量预报(英文)

It is essential to establish the water resources exploitation and utilization planning,which is mainly based on recognizing and forecasting the water consumed structure rationally and scientifically.During the past 30 years(1980-2009),mean annual precipitation and total water resource of Beijing have decreased by 6.89% and 31.37% compared with those perennial values,respectively,while total water consumption during the same period reached pinnacle historically.Accordingly,it is of great significance for the harmony between socio-economic development and environmental development.Based on analyzing total water consumption,agricultural,industrial,domestic and environmental water consumption,and evolution of water consumed structure,further driving forces of evolution of total water consumption and water consumed structure are revealed systematically.Prediction and discussion are achieved for evolution of total water consumption,water consumed structure,and supply-demand situation of water resource in the near future of Beijing using Time Series Forecasting Method.The purpose of the endeavor of this paper is to provide scientific basis for the harmonious development between socio-economy and water resources,for the establishment of rational strategic planning of water resources,and for the social sustainable development of Beijing with scientific bases.     

风向变化特征在季风模拟评估中的应用

作者抓住季风风向具有季节性反转这一最本质的特征,引入了“有向转角”的新概念,它与传统盛行风夹角的概念不同,能够反映风向逐日变化的方向性和旋转角度的大小。用欧拉观点揭示了季风风矢量随时间演变的旋转特点, 体现了季风风向独具特色的季节演变过程。同时,发现不同地区风向的季节循环有6种基本类型:（I）先顺时针后逆时针旋转、（II）先逆时针后顺时针旋转、（III）完全顺时针旋转、（IV）完全逆时针旋转、（V）风向稳定型和（VI）风向变化不稳定型。且季风风向的季节性反转主要通过前四种旋转方式来实现。分析了这6种风向变化型的全球分布特征,研究了它们与大气环流系统演变的联系。并进一步将“有向转角” 概念用于IPCC第四次评估报告AMIP试验8个模式的模拟评估,结果表明,这一概念的引入能从逐日变化的角度凸显风向变化过程,不仅能够客观反映模式模拟季风风向逐日变化的动力过程以及风矢量旋转方式的全球分布,还能体现模式对大气环流系统季节演变的表征能力。研究还发现在这8个模式中,大多数模式基本能把风矢量旋转方式的全球分布形式模拟出来,但对于季风区风矢量旋转方式的模拟还有待于进一步提高。     

近50年来中国季节性冻土与短时冻土的时空变化特征

在对中国冻土气象观测资料整理和分析的基础上, 研究了中国冻土分布的时空演变规律。主要分析了中国冻土分布的季节变化、冻土深度的空间变化, 以及冻结日期、解冻日期、冻结时间长度的空间分布特征, 同时也分析了以上各要素的时间变化特征。结果表明: 中国冻土分布广泛, 在我国东部的长江以北地区、西北地区及青藏高原地区均有分布; 其中季节性冻土具有显著的年内变化特征, 冻结一般从秋季开始, 冬末春初冻结的面积和深度达到最大, 春季逐渐开始融化, 夏季冻结的面积和厚度达到最小; 冻土的冻结过程和融化过程表现出各自不同的特征, 整个中国地区冻土的融化过程所持续的时间比冻结持续的时间长, 也更为复杂, 这与地形及土壤特性有着密切的关系; 近几十年来, 在全球变暖背景下, 中国冻土主要表现为最大冻土深度减小, 冻结日期推迟, 融化日期提前, 冻结持续期缩短, 以及冻土下界上升的总体退化趋势, 冻土的主要转型时期发生在20世纪80年代中期。     

Tectonics of the offshore Red River Fault recorded in the junction of the Yinggehai and Qiongdongnan Basins

Science China Earth Sciences - The Red River Fault, which originated from the southeastern margin of the Tibetan Plateau, has a great significance for obtaining a further understanding of the...     

Discovery of six high-redshift quasars with the Lijiang 2.4 m telescope and the Multiple Mirror Telescope

Quasars with redshifts greater than 4 are rare, and can be used to probe the structure and evolution of the early universe. Here we report the discovery of six new quasars with i-band magnitudes brighter than 19.5 and redshifts between 2.4 and 4.6 from spectroscopy with the Yunnan Faint Object Spectrograph and Camera (YFOSC) at the Lijiang 2.4 m telescope in February, 2012. These quasars are in the list of z > 3.6 quasar candidates selected by using our proposed J K/i Y criterion and the photometric redshift estimations from the SDSS optical and UKIDSS near-IR photometric data. Nine candidates were observed by YFOSC, and five among six new quasars were identified as z > 3.6 quasars. One of the other three objects was identified as a star and the other two were unidentified due to the lower signal-to-noise ratio of their spectra. This is the first time that z > 4 quasars have been discovered using a telescope in China. Thanks to the Chinese Telescope Access Program (TAP), the redshift of 4.6 for one of these quasars was confirmed by the Multiple Mirror Telescope (MMT) Red Channel spectroscopy. The continuum and emission line properties of these six quasars, as well as their central black hole masses and Eddington ratios, were obtained.     

Observations of Giant Pulses of the Crab Pulsar

The Crab Pulsar was observed at 1540 MHz with the 25m radio telescope at Urumqi with a filterbank de-dispersion backend. A total of 2436 giant pulses with pulse energies larger than 4300 Jy μs were detected in two observing sets. All of these giant pulses are located in the main pulse (MP) and inter pulse (IP) windows of the average profile of the Crab Pulsar. The ratio of the numbers of giant pulses detected in the IP and MP windows is about 0.05. Our results show that, at 1540 MHz, the emission in the IP is contributed by giant and normal pulses, while that in the MP is almost dominated by giant pulses. The distribution of energy of the 2436 giant pulses at 1540 MHz can be described by a power-law with index α=3.13±0.09. The intrinsic threshold of giant pulse energy in the MP window is about 1400 Jy μs at 1540 MHz.