The　Dynamical　Influence　of　Land－Sea　Contrast　and　Sea　Surface　Temperature　on　Intraseasonal　Oscillation　in　Tropical　Atmosphere     

Yang Yan  Zhu Baozhen 《大气科学进展》1995,12(4):405-418

An equatorial β-plane model which includes realistic non-uniform land-sea contrast and the underlying surface temperature distribution is used to simulate the 30-60 day oscillation (LFO) processes in tropical atmosphere, with emphasis on its longitude-dependent evolution and convective seesaw between Indian and the western Pacific oceans.The model simulated the twice-amplification of the disturbances over Indian and the western Pacific oceans while they are travelling eastward. It reproduced the dipole structure caused by the out-of-phase oscillation of the active centres in these two areas and the periodical transition between the phases of LFO. It is suggested that the convective seesaw is the result of interaction of the internal dynamics of tropical atmosphere with the zonally non-uniform thermal forcing from underlying surface. The convective activities are suppressed over Indonesia mari-time continents whilst they are favoured over the Indian Ocean and western Pacific warm waters, so there formed two active oscillation centres. The feedback of convection with large-scale flow slows down the propagation of disturb-ances when they are intensifying over these two areas, therefore they manifest a kind of quasi-stationary component to favor the ‘dipole’ structure. Whereas the disturbances weaken and speed up over the eastern Pacific cold water re-gion due to the interaction of sensible heating and evaporation with perturbational wind. Therefore the two major centers just show out-of-phase oscillation during onecycle around the latitudinal beltBy introducing the SST anomalies in El Ni?o and La Ni?a years into the surface temperature, we also show that they have significant influence on LFO processes. In an anomalously warm year, the LFO disturbances dissipate more slowly over the central-eastern Pacific region and can travel farther eastward; whilst in an anomalously cold year, the opposite is true.  相似文献   

Interannual variability of the convective activities associated with the east asian summer monsoon obtained from tbb variability   总被引：5，自引：0，他引：5  

Ren Baohu  Huang Ronghui 《大气科学进展》1999,16(1):77-90

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On seismic strengthening area before strong and great shocks and its mechanism   总被引：1，自引：0，他引：1  

宋治平  梅世蓉  尹祥础 《地震学报(英文版)》1999,12(3):298-305

IntroductionI.thasbeenpayingattentiontotheanomalousphenomenonbyseismologiststhattheearthquakeactivityoftenstrengthensinacertainspaceandduringacertaintimearoundthesourceareabeforeastrongearthquake.Mogi(1969)pointedoutthataringdistributiveareaofthestrengthenedearthquakeactivityoftenappearsaroundthesourcearea10to20yearsbeforegreatshock,whichcalledaringphenomenon(or"doughnut").Afterthat,otherscholarsreportedinsuccessionthatringdistributionofearthquakeactivityoccurredbeforeastrongertquakeorevenbefo…  相似文献   

Distribution of ionospheric O<Superscript>+</Superscript> ion in synchronous altitude region     

Jiankui?Shi?Email author  Zhenxing?Liu  Zhang?T.?L.  Jianshan?Guo  Manlian?Zhang  Sheping?Shang  Xigui?Luo 《中国科学D辑(英文版)》2003,46(10):986-993

Based on satellite observation data, using dynamics equation, the ionospheric O⁺ ion’s distribution in the synchronous altitude region for different geomagnetic activity indexK _p is studied by theoretical modeling and numerical analyzing, and semi-empirical models for the O⁺ ion’s density and flux versus longitude in the synchronous altitude region for differentK _p are given. The main results show that in the synchronous altitude region: (i) The O⁺ ion’s density and flux in day-side are larger than those in nightside. (ii) With longitude changing, the higher the geomagnetic activity indexK _p is, the higher the O⁺ ion’s density and flux, and their variation amplitude will be. The O⁺ ion’s density and flux whenK _{p ≥} 6 will be about ten times as great as that whenK _p = 0. (iii) WhenK _p = 0 orK _{p ≥} 6, the O⁺ ion’s density reaches maximum at longitudes 120° and 240° respectively, and minimum in the magnetotail. WhenK _p = 3−5, the O⁺ ion’s density gets to maximum at longitude 0°, and minimum in the magnetotail. However, the O⁺ ion’s flux reaches maximum at longitude 120° and 240° respectively, and minimum in the magnetotail for anyK _p value.  相似文献   

“地球空间双星探测计划”及其与全球环境变化的关系          下载免费PDF全文

刘振兴 《第四纪研究》2002,22(6):500-509

本文论述了“地球空间双星探测计划”(简称双星计划)及其与全球环境变化的关系。地球空间双星探测计划包括两颗小卫星,分别运行于目前国际上地球空间探测卫星尚未覆盖的近地赤道区和近地极区。双星计划的主要科学目标是用高分辨率的仪器在近地空间的主要活动区探测场和粒子的时空变化;研究磁层空间暴(磁层亚暴、磁暴和磁层粒子暴)的触发机制及其对太阳活动和行星际扰动的响应过程;建立地球空间环境的动态模式。为了实现科学目标,赤道区卫星和极区卫星上各载有8台探测仪器。近地赤道区卫星的轨道是:近地点550km左右,远地点60000km左右,倾角约28.5°;近地极区卫星的轨道是:近地点700km,远地点40000km,倾角约90°。为了使双星计划与欧洲空间局ClusterII卫星相配合,赤道区卫星计划于2003年6月发射,极区卫星计划于2003年12月发射。双星计划与ClusterII卫星相配合,可形成地球空间6点探测计划,这将成为21世纪初国际上重要的地球空间探测计划。本文概要讨论了双星计划与地球系统各圈层的关系,包括与大气圈、生物圈、地球内部各圈层及全球环境变化的关系。  相似文献   

A comparison between photospheric and chromospheric quiet-Sun magnetograms     

Zhang  Mei  Zhang  Hongqi 《Solar physics》2000,194(1):19-28

Photospheric (Fei 5324.19 Å line) and chromospheric (H line) magnetic fields in quiet-Sun regions have been observed in the solar disk center by using the vector video magnetograph at Huairou Solar Observing Station of Beijing Astronomical Observatory. Observational results show that the quiet-Sun magnetic elements in the solar photosphere and chromosphere present similar magnetic structures. Photospheric and chromospheric magnetograms show corresponding time variations. This suggests that the magnetic fields in quiet-Sun regions present different 3-D magnetic configurations compared to those in solar active regions.  相似文献   

Diffusive wave solutions for open channel flows with uniform and concentrated lateral inflow     

P. Fan  J.C. Li 《Advances in water resources》2006

The diffusive wave equation with inhomogeneous terms representing hydraulics with uniform or concentrated lateral inflow into a river is theoretically investigated in the current paper. All the solutions have been systematically expressed in a unified form in terms of response function or so called K-function. The integration of K-function obtained by using Laplace transform becomes S-function, which is examined in detail to improve the understanding of flood routing characters. The backwater effects usually resulting in the discharge reductions and water surface elevations upstream due to both the downstream boundary and lateral inflow are analyzed. With a pulse discharge in upstream boundary inflow, downstream boundary outflow and lateral inflow respectively, hydrographs of a channel are routed by using the S-functions. Moreover, the comparisons of hydrographs in infinite, semi-infinite and finite channels are pursued to exhibit the different backwater effects due to a concentrated lateral inflow for various channel types.  相似文献   

A Statistical Investigation of the Earthquake Predictions Using LURR     

Keyin Peng  Xiangchu Yin  Lang-Ping Zhang 《Pure and Applied Geophysics》2006,163(11-12):2353-2362

In terms of the spatial scanning of LURR (Load-Unload Response Ratio), we have been predicting the seismic tendency within the next year for the mainland of China from 1995 to 2003. In order to make the quantitative retrospective assessment of LURR method, we compare the results with Poisson null hypothesis. The results show that the prediction by LURR method is much better than Poisson hypothesis.  相似文献   

岩石中微生物学研究的分子生物学技术——中国大陆科学钻探（CCSD）微生物研究     

李光玉王远亮  董海良东秀珠 董志扬 《岩石学报》2006,22(7):2107-2111

本文介绍了中国大陆科学钻探（CCSD）微生物学研究中所建立起来的分子生物学技术，即环境基因组DNA提取、16SrDNA分析、Real-timePCR技术和磷脂酸分析技术。另外探索了防污染的手段以及监测方法，并介绍了我们以这种方法对CCSD的微生物学研究所得到的一些初步结果。  相似文献   

快速精密星历替代精密星历定位的初步研究   总被引：3，自引：1，他引：3       下载免费PDF全文

尹继尧  徐平  吴培稚 《地震工程学报》2006,28(1):36-41

由于GPS精密定位所需的IGS精密星历要在两周以后才能得到,因而利用两天后即可得到的快速精密星历、12小时后得到的超快速精密星历代替精密星历是GPS应用于地震短临预测的一个重要条件。本文利用北京市全球定位综合应用服务系统中五个GPS连续观测站一年半的数据,分别用三种星历进行精密定位计算,得到了小规模网中快速精密星历一般可以代替精密星历进行精密定位计算的结果。  相似文献