成人学前教育专业教学存在的若干问题及解决策略——以美术教学为例     

张菡 《吉林气象》2015,(2):90-93

本文旨在为成人学前教育美术专业的教师改进教学提供借鉴。成人学前教育美术专业教学中存在诸多问题:美术课程设置不够完善、美术师资力量不强、教学资源相对不足、教学内容与方法还不令人满意、学生的自学能力较弱等。针对这种现状,本文拟就所存在的问题作以探讨分析,进而提出相应的改进策略。  相似文献   

CORRELATION ANALYSIS OF THE WESTERN PACIFIC SUBTROPICAL HIGH AND EASTERN ASIAN SUMMER MONSOON SYSTEM BASED ON FUZZY SYSTEMS AND DYNAMICAL MODEL INVERSION FORECAST     

洪梅  张韧  阎恒乾  葛晶晶 《热带气象学报(英文版)》2015,21(S1):34-45

Based on the adaptive network fuzzy inference system (ANFIS), methods to filter out the noise of impact factors from the main signal are discussed. Focusing on the abnormal weather conditions in 2010, we use the delay-relevant method to analyze the five members of the summer monsoon system that had the largest effect on the subtropical high anomalies from the observational data. ANFIS is suitable for research and simulation of subtropical highs that are difficult to describe accurately with dynamics, allowing the effect of five factors on the subtropical high anomalies to be examined. Our results show that the Mascarene cold high, the Indian monsoon latent heat flux, and the South China Sea monsoon trough had the largest effect on the subtropical high anomalies. Diagnostic analysis, with genetic algorithms (GA) and dynamical reconstruction theory, reconstructed the nonlinear dynamical model of the subtropical high and its main factors objectively and accurately from the sequence of observations in 2010. Furthermore, a dynamically extended forecast experiment is performed. The forecasts for the subtropical high area index, the Mascarene cold high index, the Indian monsoon latent heat flux, and the South China Sea monsoon trough index all show a strong short-term effect over less than 25 days. The forecasting trend is accurate, and the error rate is no more than 7%. Our results provide new insight and methods for research on the association between the western Pacific subtropical high and the East Asian summer monsoon system, and for the prediction of the western Pacific subtropical high index.  相似文献   

IMPACT OF SSTA OF SOUTHERN HEMISPHERE ON FLOOD SEASON PRECIPITATION ANOMALIES IN YUNNAN     

杨竹云  杨素雨  严华生  张瑾文 《热带气象学报(英文版)》2015,21(3):255-264

Based on the reanalysis data of monthly mean global SST and wind from the NCEP/NCAR and the observation data of rain seasons in 124 stations of Yunnan province from 1961 to 2006, we applied the analytical methods of correlation analysis and composite analysis and a significance testing method to two sets of samples of average differences. The goal is to investigate into the influence of the Southern Hemispheric (SH) SST on the summer precipitation in Yunnan from January to May so as to identify the key time and marine regions. Physical mechanisms are obtained by analyzing the influence of sea level wind and the key marine regions on the precipitation during Yunnan’s rain season. Results show that there is indeed significant relationship between the SST in SH and summer precipitation in Yunnan. The key areas for influencing the summer precipitation are mainly distributed in a region called “West Wind Drift” in the SH, including the Southeast Indian, southern Australia, west coast of eastern Pacific off Chile, Peru and the southwest Atlantic Magellan. Besides, the most significant marine region is the west coast of Chile and Peru (cold-current areas of the eastern Pacific). Diagnostic analysis results also showed that monsoons in the Bay of Bengal, a cross-equatorial flow in the Indian Ocean near the equator and southwest monsoon in India weaken during the warm phase of the Peruvian cold current in the eastern Pacific. Otherwise, they strengthen.  相似文献   

H2CO and HI 10α survey toward UCHII regions     

Xiao-Hong Han  Jian-Jun Zhou  Jarken Esimbek  Gang Wu  Ming-Fei Gao 《中国天文和天体物理学报》2011,11(2)

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铜陵地区晚古生代岩浆活动的发现：来自凤凰山岩体ZK66钻孔岩心辉绿岩锆石U–Pb定年的证据          下载免费PDF全文

吴才来董树文  王次松高前明  闫永涛李 翔 郜源红 雷 敏秦海鹏  李名则刘春花 《中国地质》2013,40(3):715-729

凤凰山花岗闪长岩是铜陵地区出露面积最大的岩体,约10 km2,属高钾钙碱性系列.位于该岩体西北角的朱家山附近ZK66钻孔揭示,岩体超覆于三叠纪碳酸盐岩地层之上.除在浅部见到花岗闪长岩之外,深部主要见到晚泥盆世-二叠纪地层.特别是在石炭纪大理岩中见到辉绿岩和花岗斑岩,其锆石LA-ICP-MS U-Pb年龄分别为304 Ma和132 Ma,证明本区存在晚古生代岩浆活动,而中生代花岗质岩浆活动可能持续到132 Ma.晚石炭世辉绿岩的发现,说明该时期海底是一种拉张环境,海底喷流作用可能与岩浆活动有密切的成因关系,为该时期形成大型矿床奠定了基础.  相似文献   

耀变体3C 273在2～10keV的光变特性研究     

吴霄  刘智敏  闫大海  包昆森  戴本忠 《天文学报》2010,51(3)

从RXTE(Rossi X-ray timing explorer)观测原始数据出发,分析了耀变体3C 273在X射线波段2～10 keV从1996年2月2日(MJD 50115)到2007年8月27日(MJD 54339)的数据.一共得到了1 010次观测数据的光子谱指数和相应的流量,平均每次观测时间为1 666.76 s.通过分析3C 273在观测期间2～10 keV硬X射线的能谱变化及光变行为,发现在2000年2月,2003年3、4月,2004年2、3、7月,2006年及2007年,其光子谱指数Γ与流量lgF_(2～10 keV)存在显著反相关.在1999年和2000～2007年观测期间,Γ与lgF_(2～10 keV)月平均行为也同样存在显著反相关.对整个观测期间的光变行为作定量的分析,发现几次较大的光变,并在部分光谱拟合中发现Fe发射线存在的证据,其平均宽度为93.85±21.49 eV.通过分析光变强度与Fe发射线特性,发现3C 273同时具有耀变体与Seyfert星系的一些性质.  相似文献   

The effect of metallicity on the minimum mass ratio of W Ursae Majoris-type systems     

Dengkai Jiang  Zhanwen Han  Cheng Liu  Jiancheng Wang  Lifang Li 《Astrophysics and Space Science》2010,329(1-2):283-286

According to the prevenient theoretical study, the minimum mass ratio for tidal stability of W Ursae Majoris (W UMa) systems is q _min?=(M ₂/M ₁)～0.071–0.078. However, the mass ratios of some observed W UMa binaries are smaller than the theoretical minimum mass ratio. Using Eggleton’s stellar evolution code, we study the effects of metallicity and evolution on the minimum mass ratio of W UMa systems (M ₁=1.2M _⊙). We assume that $k_{1}^{2}=k_{2}^{2}$ for the component’s dimensionless gyration radii and that the contact degree is about 70 per cent. We find that the dynamical stability of W UMa binaries depends on the metallicity of W UMa systems. For the W UMa systems at age = 0 Gyr, the distribution of the minimum mass ratio has a fairly wide range, from 0.083 to 0.064, with the metallicity range from Z=0.0001 to 0.03. W UMa systems with Z=0.01 have the smallest value of the minimum mass ratio, which is about 0.064. The existence of low-q systems can be explained partly by the dependence of the dimensionless gyration radius on the metallicity. In addition, the dependence of the minimum mass ratio on the evolution, as suggested by previously work, is confirmed.  相似文献   

Contribution of close double white dwarfs to the Galactic gravitational wave foreground     

Jinzhong Liu  Yu Zhang  Zhanwen Han  Fenghui Zhang 《Astrophysics and Space Science》2010,329(1-2):297-303

This paper provides new detailed specifics and characteristics of the close double white dwarfs (CDWDs) LISA foreground noise floor using the newest information on the astrophysics with binary population algorithms, which were judged to satisfy the observations. We use the binary population synthesis approach of CDWDs in combination with the latest findings of synthesis models from Han (Mon. Not. R. Astron. Soc. 296:1019, 1998), here, specifically formation by the three evolutionary channels of (a) stable Roche lobe overflow plus common envelope (RLOF?+?CE), (b) CE plus CE, (c) exposed core plus CE. We collect resulting CDWDs in the frequency range of 10^?8 Hz to 10^?2 Hz and compare strength and number statistics per resolvable frequency bin to derive the properties of the noise floor and the nature of possible outliers that may become individually resolvable. We find resolvable outliers to be solely produced by CE?+?CE evolution; the other two channels contribute only to the unresolvable foreground noise. Within the CE?+?CE evolution a detailed look into the chemical buildup of the stars reveals dominantly double helium (He?+?He) WDs or carbon-oxygen CO?+?He WDs.  相似文献   

The light-weighted age and metallicity of Galactic globular clusters     

Yu Zhang  Fenghui Zhang  Zhanwen Han  Jinzhong Liu 《Astrophysics and Space Science》2010,329(1-2):255-260

Spectra synthesis is entering a new era with the availability of large and high-quality spectroscopic data and full spectrum fitting methods. Establishing the reliability whether the STARLIGHT code (a full spectrum fitting code, Cid Fernandes et al. (Mon. Not. R. Astron. Soc. 358:363, 2005)) is suitable to study the properties of various types of galaxies is vital to galaxy study. In testing this possibility, Galactic globular clusters (GCs) provide an excellent medium. Taking the 40 Galactic GCs as an example in our work, we analyze their integrated spectra from Schiavon et al. (Astrophys. J. Suppl. 160:163, 2005) and obtain their mixtures of stellar populations that best represents their composite nature. Through analyzing the distributions of stellar ages and metallicities respectively, we find that the stellar metallicity distribution is centered at a low value and the stellar age distribution is very scattered. To compare with the literature, we also calculate the light-weighted ages and metallicities of GCs, and we find that the light-weighted metallicities agree with the literature, while the light-weighted ages are lower than those of the literature. This demonstrates that STARLIGHT can be used to obtain the metallicities of GCs.  相似文献   

Habitable zones and UV habitable zones around host stars     

Jianpo Guo  Fenghui Zhang  Xianfei Zhang  Zhanwen Han 《Astrophysics and Space Science》2010,325(1):25-30

Ultraviolet radiation is a double-edged sword to life. If it is too strong, the terrestrial biological systems will be damaged. And if it is too weak, the synthesis of many biochemical compounds cannot go along. We try to obtain the continuous ultraviolet habitable zones, and compare the ultraviolet habitable zones with the habitable zones of host stars. Using the boundary ultraviolet radiation of ultraviolet habitable zone, we calculate the ultraviolet habitable zones of host stars with masses from 0.08 to 4.00 M _⊙. For the host stars with effective temperatures lower than 4,600 K, the ultraviolet habitable zones are closer than the habitable zones. For the host stars with effective temperatures higher than 7,137 K, the ultraviolet habitable zones are farther than the habitable zones. For a hot subdwarf as a host star, the distance of the ultraviolet habitable zone is about ten times more than that of the habitable zone, which is not suitable for the existence of life.  相似文献