江苏省植物气候生产力时空演变特征   总被引：3，自引：2，他引：1  

肖卉  沈瑱  唐红昇  程婷 《气象科学》2008,28(Z1)

根据江苏省59站1960-2006年年平均气温、降水量资料,采用Thornthwaite Memo-riai模型计算了江苏植物气候生产力(TSPV),用EOF等统计方法分析了TSPV时空分布变化特征.结果表明:江苏省总体气候生产力水平呈南高北低的状态,随纬度增高而降低;北部气候生产力近年来不断增长,南部则较为平稳;EOF分析结果表明江苏的气候生产力主要有全省一致、苏南和苏北相反、江淮为中心等分布型.  相似文献   

CA-FCM方案与其它几种人工增雨评估方案的比较   总被引：3，自引：0，他引：3  

房彬  肖辉  班显秀 《气象科技》2008,36(5)

对河南省12次飞机增雨作业,分别采用作业区域趋势对比双比分析评估方案、区域趋势相关回归分析方案、区域趋势协变量多元回归分析方案、浮动对比区历史回归分析方案(FCM)、以降水量为协变量的CA-FCM(Cluster-Analysis-based Floating Contro historical regression Method)方案和以降水量和整层大气可降水量为协变量的CA-FCM方案进行效果评估,均得到大于15%的相对增雨量.对结果比较分析表明:协变量由降水量和整层大气降水量两个组成的CA-FCM方案,由于采用了聚类分析提高了对比区和影响区相关系数和引入了整层大气可降水量作为协变量提高了作业区自然降水量估计值的准确性,从而比其它评估方案效果更好.  相似文献   

气候变化适应行动进展及对我国行动策略的若干思考     

居煇  韩雪 《气候变化研究进展》2008,4(5):257-260

 巴厘岛会议,即《联合国气候变化框架公约》（简称《公约》）第13次缔约方会议,明确了将气候变化适应和减缓并重的立场,并对适应工作进行了一系列的安排和部署。通过介绍《公约》下适应认识的发展过程,阐述了巴厘岛会议针对适应行动的一些进展,讨论了我国在适应方面可开展的行动和关注的领域。分析认为,目前适应已成为和减缓并重的关注议题,适应行动的呼声越来越强烈,但行动的落实还需要经过漫长的过程,适应基金募集和分配在发达国家和发展中国家之间、发展中国家内部也将有一个艰难而激烈的谈判交锋。  相似文献   

利用VB语言开发县级MICAPS 2.0资料本地化接收系统     

虎莹  王志强  田辉 《气象与环境科学》2008,31(Z1)

针对县级无法及时、完全接收卫星资料的问题,利用VB语言开发了县级MICAPS2.0资料本地化接收系统,使县级气象台站能够共用地(市)级的卫星单收站接收的资料.  相似文献   

双流冬草莓低温冻害天气特征及防冻措施探讨   总被引：1，自引：0，他引：1  

罗琴  于成  蔡霞  叶丽君  肖楷  祝康 《高原山地气象研究》2008,28(3):72-75

双流县作为我国最大的冬草莓生产基地,低温冻害是冬季生产关键期的主要气象灾害。本文对2005年初低温冻害进行了分析,归纳出了双流县冬草莓低温冻害的发生规律及冻害临界温度指标,并提出了具体的防冻措施。  相似文献   

Shock waves in the large-scale structure of the Universe     

Dongsu Ryu  Hyesung Kang 《Astrophysics and Space Science》2009,322(1-4):65-70

Cosmological shock waves are induced during hierarchical formation of large-scale structure in the universe. Like most astrophysical shocks, they are collisionless, since they form in the tenuous intergalactic medium through electromagnetic viscosities. The gravitational energy released during structure formation is transferred by these shocks to the intergalactic gas as heat, cosmic-rays, turbulence, and magnetic fields. Here we briefly described the properties and consequences of the shock waves in the context of the large-scale structure of the universe.  相似文献   

Observational Study of a Peculiar Solar Limb Event Occurred on 11 January 2002     

Hui Li  Jianqi You 《Solar physics》2009,258(1):89-104

On 11 January 2002, using the Multi-channel Infrared Solar Spectrograph (MISS) at the Purple Mountain Observatory (PMO), we obtained Hα, Ca ii 8542 Å and He i 10?830 Å spectra and slit-jaw Hα images of a peculiar solar limb event. A close resemblance of its intensity to that of a small flare and the GOES X-ray flux indicates that it was an active prominence. However, its morphological evolution and velocity variation were different from general typical active prominences, such as limb flares, post-flare loops, surges and sprays. It started with the ejection of material from the flare site. In the early phase, the ejecta was as bright as a limb flare and kept rising until reaching the height of (8????10)×10⁴ km at an almost constant velocity of 91.7 km? s ^?1 with its lower part always connected to the solar surface. EUV images in 195 Å show similar structure as in the Hα line, indicating the coexistence of plasmas with temperatures differing by more than two orders of magnitude. Later some material started to fall back to another bright area on the solar surface. The falling material did not show the collimated structure of surges or the arc structure of flaring arches. A red-shift velocity of more than 200 km? s ^?1 was detected in a bright point close to the outer edge of the closed loop system formed later, which dispersed in a few minutes and became a part of the newly formed large loop. The ejected material did not leave the sun, indicating that the magnetic reconnection was not sufficient to remove the overlying field lines during the process. The spectral line profiles showed large widths and variable velocities, and therefore the line-pair method is not applicable to this event for the estimation of physical parameters.  相似文献   

利用窄线宽激光测量锶原子束速率分布     

赵亚楠  吴慧  常宏  张首刚 《时间频率学报》2009,32(1):1-5

利用多普勒频移效应,通过线宽2MHz窄线宽激光与锶原子束在大角度作用下的荧光信号分析,测量了锶原子束速率分布。比较和分析表明,理论结果与实验结果符合较好。  相似文献   

Flare-induced signals in polarization measurements during the X2.6 flare on 2005 January 15     

Meng Zhao  Jing-Xiu Wang  Sarah Matthews  Ming-De Ding  Hui Zhao  Chun-Lan Jin 《中国天文和天体物理学报》2009,9(7)

Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two questions: can we distinguish the flare-induced signals from real magnetic changes during flares, and what we can learn about flare energy release from the flare-induced signals? We select the X2.6 flare that occurred on 2005 January 15, for further study. The flare took place in NOAA active re-gion (AR) 10720 at approximately the central meridian, which makes the interpretation of the vector magnetograms less ambiguous. We have identified that flare-induced signals during this flare appeared in six zones. The zones are located within an average distance of 5 Mm from their weight center to the main magnetic neutral line, have an average size of (0.6±0.4)×1017 cm2, duration of 13±4 min, and flux density change of 181±125 G in the area of reversed polarity. The following new facts have been revealed by this study: (1) the flare-induced signal is also seen in the transverse magnetograms but with smaller magnitude, e.g., about 50 G; (2) the flare-induced signal mainly manifests itself as apparent polarity reversal, but the signal starts and ends as a weakening of flux density; (3) The flare-induced signals appear in phase with the peaks of hard X-ray emission as observed by the Ramaty High Energy Solar Spectroscopic lmager (RHESSI), and mostly trace the position of RHESSI hard X-ray footpoint sources. (4) in four zones, it takes place cotemporally with real magnetic changes which persist after the flare. Only for the other two zones does the flux density recover to the pre-flare level immediately after the flare.The physical implications of the flare-induced signal are discussed in view of its relevance to the non-thermal electron precipitation and primary energy release in the flare.  相似文献   

Investigation of fractal distribution law for the trace number of random and grouped fractures in a geological mass   总被引：1，自引：0，他引：1  

Yangsheng Zhao  Zengchao Feng  Weiguo Liang  Dong Yang  Yaoqin Hu  Tianhe Kang 《Engineering Geology》2009,109(3-4):224-229

A fractal study method of the number of geological mass fractures is introduced in detail in this paper. Three main aspects of the problem were studied: (1) The random distribution of fractures in a geological mass was in good agreement with the fractal law. The size scale of the studied geological mass ranged from 2400 m to 1 mm for the length of each side, and the geological mass samples were taken from 13 coal areas in China. (2) The geological mass fractures were evidently directional and anisotropic, having originated from tectonic movement. Observation and statistics for the data from the Xuangang, Fenxi and Dongshan coal areas in Shanxi, China, demonstrated that the fracture distribution of each group, classified by the strike of the strata, still follow the fractal law, even though the fractal dimension varies to a certain extent with different strikes. (3) The sedimentary strata containing the coal seams, as a geological mass, underwent almost similar tectonic movements in their geological history. The mechanical experiments on geological mass samples from Fenxi and Jiexiu in Shanxi demonstrated that the fractal dimension of the number of fractures in the same strata is in good power function with the product of strength and elastic modulus. The larger the product of the strength of the elastic modulus is, the larger is the fractal dimension, and vice versa.  相似文献