k=6,7,8,9的一类新几乎差族

C.Ding和J.Yin推广了几乎差集,定义了新的几乎差族的概念.通过有限域中分圆类的方法给出了几乎差族新的构造方法,并得到了k=6,7,8,9的一类新的几乎差族.     

2010年6月中下旬南方暴雨过程变形场作用分析

利用常规原始报文资料,采用基于Lanczos窗口滤波器的合成分析方法,对2010年6月13-27日的形势场、物理量进行合成分析,计算并分析了低空合成风场的总变形.结果表明:500 hPa大陆中、高纬地区存在一“Ω”形类阻塞高压,西北冷空气从其东部源源不断向长江及以南地区输送,与副热带高压西北侧的西南暖湿气流在我国南方地区交汇.700、850 hPa大陆高压与西太平洋副热带高压之间形成的鞍型场,位于长江以南地区,鞍型场鞍点附近及其东部膨胀轴是暴雨发生的主要区域.在南方地区上空200 hPa西北气流辐散产生的抽吸作用,对这次长时间、高强度的降水起了重要作用.发生在鞍型场和切变线上的低空中尺度气旋,是造成暴雨的重要天气系统.鞍型场膨胀轴附近,总变形最大,其位置、走向均与雨带基本一致,有利于锋生和中尺度气旋形成.低空冷暖气流交汇区域形成低空强θse梯度,在垂直剖面图上,等θse线呈现十分倾斜状态,该区域强θse水平梯度与低空总变形、正涡度区一致,可能是特大暴雨发生的重要因素.     

Contributions of individual variation in temperature, solar radiation and precipitation to crop yield in the North China Plain, 1961–2003

An understanding of the relative impacts of the changes in climate variables on crop yield can help develop effective adaptation strategies to cope with climate change. This study was conducted to investigate the effects of the interannual variability and trends in temperature, solar radiation and precipitation during 1961–2003 on wheat and maize yields in a double cropping system at Beijing and Zhengzhou in the North China Plain (NCP), and to examine the relative contributions of each climate variable in isolation. 129 climate scenarios consisting of all the combinations of these climate variables were constructed. Each scenario contained 43 years of observed values of one variable, combined with values of the other two variables from each individual year repeated 43 times. The Agricultural Production Systems Simulator (APSIM) was used to simulate crop yields using the ensemble of generated climate scenarios. The results showed that the warming trend during the study period did not have significant impact on wheat yield potential at both sites, and only had significant negative impact on maize yield potential at Beijing. This is in contrast with previous results on effect of warming. The decreasing trend in solar radiation had a much greater impact on simulated yields of both wheat and maize crops, causing a significant reduction in potential yield of wheat and maize at Beijing. Although decreasing trends in rainfed yield of both simulated wheat and maize were found, the substantial interannual variability of precipitation made the trends less prominent.     

Fast compression and reconstruction of astronomical images based on compressed sensing

With the fast increase in the resolution of astronomical images, the question of how to process and transfer such large images has become a key issue in astronomy. We propose a new real-time compression and fast reconstruction algorithm for astronomical images based on compressive sensing techniques. We first reconstruct the original signal with fewer measurements, according to its compressibility. Then,based on the characteristics of astronomical images, we apply Daubechies orthogonal wavelets to obtain a sparse representation. A matrix representing a random Fourier ensemble is used to obtain a sparse representation in a lower dimensional space. For reconstructing the image, we propose a novel minimum total variation with block adaptive sensing to balance the accuracy and computation time. Our experimental results show that the proposed algorithm can efficiently reconstruct colorful astronomical images with high resolution and improve the applicability of compressed sensing.     

Photometric Studies of Twelve Deep, Low-mass Ratio Overcontact Binary Systems

The formations of the blue straggler stars and the FK Com-type stars are unsolved problems in stellar astrophysics. One of the possibilities for their formations is from the coalescence of W UMa-type overcontact binary systems. Therefore, deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars are a very important source to understand the phenomena of Blue Straggler/FK Com-type stars. Recently, 12 W UMa-type binary stars, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, V410 Aur, XY Boo, SX CrV, QX And, GSC 619-232, and AH Cnc, were investigated photometrically. Apart from TV Mus, XY boo, and GSC 619-232, new observations of the other 9 binaries were obtained. Complete light curves of the 10 systems, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, GSC 619-232, V410 Aur, XY Boo, and AH Cnc, were analyzed with the 2003 version of the W-D code. It is shown that all of those systems are deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars. We found that the system GSC 619-232 has the highest degree of overcontact (f = 93.4%). The derived photometric mass ratio of V857 Her, q = 0.0653, indicates that it is the lowest-mass ratio system among W UMa-type binaries.Of the 12 sample stars, long-term period changes of 11 systems were found. About 58% (seven) of the sample binaries show cyclic period oscillation. No cyclic period changes were discovered for the other 5 systems, which may be caused by the short observational time interval or by insufficient observations. Therefore, we think that all W UMa-type binary stars may contain cyclic period variations. By considering the long-term period changes (both increase and decrease) of those binary stars, we proposed two evolutionary scenarios evolving from deep, low-mass ratio overcontact binaries into Blue Straggler/FK Com-type stars.     

溃变图的业务操作系统简介

按溃变理论［１］的不连续或非均匀信息不仅可以预测天气系统的移动性变化和转折性变化，也可以预测降水等天气现象。并已被多次历史例案和应用实践所验证。为了便于投入业务运用，我们利用数据库系统，实现了体现资料信息非均匀和不连续的广义参数在微机、填图机上的自动化处理，完成了收报、计算和填图分析的自动化。本方法体现了预报工具的改革也充分地利用了现有的资料资源     

济南市历城区土地开发整理工作纪实

0引言济南市历城区南依泰山,北靠黄河,自西汉初设县,距今已有2100多年的历史,素有“齐鲁首邑”之称,总面积1 303 km2,辖4个街道办事处、11个镇, 47个社区居委会、651个行政村。全区人口88万,土地面积13．03万hm2,其中耕地面积4．06万hm2。人均耕地约0．046 7 hm2(0．7亩),远远低于全国、全省平均水平,是典型的人多地少区域。随着社会经济的快速发展,人口的急剧增加,用地矛盾日益尖锐。作为担负着全区国土资源管理重任的职能部门,历城区国土资源局在区委、区政府和市国土资     

Rotational evolution of protoneutron stars with hyperons: spin up or not?

We study the evolution of a rigidly rotating protoneutron star (PNS) with hyperons and nucleons or solely nucleons in its core due to the escape of trapped neutrinos. As the neutrinos escape, the core nucleonic neutron star (NS) expands and the stellar rotation slows. After the neutrinos escape, the range of the spin periods is narrower than the initial one, but the distribution is still nearly uniform. A PNS with hyperons, at the late stage of its evolution, keeps shrinking and spinning up until all the trapped neutrinos escape. Consequently, the distribution of the stellar initial spin periods is skewed towards shorter periods. If the hyperonic star is metastable, its rotational frequency accelerates distinguishedly before it collapses to a black hole.     

井中地震用于陆相储层分析的几项技术

中国陆相储层分布广泛，类型复杂，横向变化大，勘探开发成本高，进行储层分析要求采用高新技术和综合利用多种方法。本文总结了在我国几个油区进行陆相储层分析的几项地震技术即：垂直地震剖面（ＶＳＰ）技术，多偏移距和井间层析成象技术以及多参数分析和综合解释技术，在适应我国经济发展的水平和现状的条件下，用以解决我国复杂的陆相油气储层分析的问题。