近44年无锡寒潮天气变化特征分析   总被引：2，自引：0，他引：2  

阮蔚琳  马志强  章志芹 《湖北气象》2007,26(2):139-143

利用无锡市1959～2002年共44a的逐日最低气温资料,分析了无锡寒潮发生的特点.分析结果表明:无锡寒潮的年发生次数有线性减少趋势;寒潮减少主要发生在10月、12月、4月.分年代看,从20世纪60年代到80年代逐年代减少,但90年代又增多.寒潮减少与降温幅度减小、最低气温升高有关,其中最低气温升高是其主要影响因素.特征区域的500 hPa高度场偏高是寒潮发生次数减少的直接原因.最后,针对多寒潮年和少寒潮年的环流特点,给出了500 hPa典型距平场特征.  相似文献   

大巴山前陆西段叠加构造变形分析及其构造应力场特征   总被引：5，自引：4，他引：5       下载免费PDF全文

施炜董树文  胡健民张忠义 刘刚 《地质学报》2007,81(10):1314-1327

大巴山前陆西段发育典型的横跨叠加褶皱,清楚地记录了自身构造演化历史,为查明大巴山前陆构造体制转换提供了非常有利的条件。本文通过野外褶皱形态分析,结合层面和断层面滑动矢量的观测,获得大巴山前陆西段中生代主要的两期挤压构造应力场,即早期(T3—J1)的构造应力场以近南北向挤压为主,大巴山地区受其控制,发生近东西向展布褶皱变形,这期构造变形与印支运动有关;晚期,即J3—K1期间,大巴山构造体制发生重大转变,本区构造应力场由近南北挤压转变为近东西向强烈挤压,大巴山发生强烈构造变形,大巴山推覆构造带以断裂活动为主,镇巴—城口—房县断裂带强烈向大巴山前陆逆掩。而大巴山前陆则以强烈的近南北向延伸的褶皱变形为主,早期近东西向褶皱遭受强烈改造,形成大巴山前陆西段较为典型的横跨叠加褶皱构造。这期构造变形是燕山运动早期活动的结果。大巴山叠加变形的研究不仅为研究中国盆—山系统变形特征提供了具体例证,而且对大巴山前陆油气勘探起重要指导作用。  相似文献   

由多个震源机制解分析民乐Ms6.1级地震前后应力场演化     

张辉  刘小凤  赵凌云 《高原地震》2007,19(3):《高原地震》-6-9,20

2003年10月25日在甘肃省民乐县和山丹县境内发生了Ms6．1与Ms5．8级地震，对震区200km范围、震前2年内发生的地震，及对震后部分余震矩张量反演得到它们的震源机制解，并对其进行统计分析得到该区的背景应力场及应力轴的整体特征，根据发震区地质构造背景和对平均应力场变化分析，寻求民乐地震的发震机制。  相似文献   

吴堡矿区横沟井田矿井充水因素评价     

杨智国  梁秀娟 《陕西地质》2007,35(1):78-83

吴堡矿区赋存着丰富的煤炭资源,但开采技术条件较复杂,其中水文地质条件复杂是影响煤炭开采的主要不利开采技术条件。本文依据横沟井田勘探资料,较全面地分析了井田水文地质条件,并着重评价了井田矿井充水因素。认为黄河水对横沟井田煤炭开采无影响;奥灰承压水对山西组煤层开采在正常地段不会造成危害,对太原组煤层开采有很大的威胁。并提出太原组煤层能否开采利用,还需进一步作详细地质勘查研究工作。  相似文献   

北太平洋风暴轴异常变化特征及其与纬向风场的关系研究   总被引：7，自引：2，他引：7       下载免费PDF全文

韩博  任雪娟  杨修群 《气象科学》2007,27(3):237-245

摘要本文通过对300 hPa5、00 hPa和850 hPa的北太平洋风暴轴(PST)的异常研究,分别提取出两个主异常模态进行比较。分析表明在三层的第一主模态都主要对应有PST异常的准10 a的周期变化;而对300 hPa和500 hPa的第二主模态,以及850 hPa的第三模态,对应有更长时间的趋势变化。进一步通过相关的分析,说明PST的异常从低层到高层的变化存在一定的一致性。通过PST与纬向风场在300 hPa的相关分析发现,两个模态与纬向风场的异常在空间上都呈同位相的分布,说明高层纬向风场异常与PST发展可能存在一种互相反馈的作用。进一步通过斜压增长率和水平两维的E-P通量矢的合成分析发现,这种反馈作用,无论从纬向风场异常所产生的环境斜压增长条件的改变,还是从平均动能与扰动动能的转化关系,都是存在的。  相似文献   

Disc structure around strongly magnetic accretors: a full disc solution with buoyancy diffusivity     

C. G. Campbell  & P. M. Heptinstall 《Monthly notices of the Royal Astronomical Society》1998,301(2):558-568

A full numerical solution is found for the effect of a strongly magnetic star on its accretion disc, for the case of magnetic buoyancy diffusion. As in the previously considered case of turbulent diffusion, the disc becomes disrupted when magnetic and viscous stresses become comparable. A magnetically induced temperature elevation leads to electron scattering opacity and radiation pressure becoming significant far from the stellar surface, with consequent viscous instability and vertical disruption of the disc. This, together with the previous turbulent case, suggests that such a disruption mechanism owing to strongly magnetic accretors is generally operable.  相似文献   

Spectroscopic observations of the eclipsing polar MN Hya (RX J0929–24)     

Gavin Ramsay  & Peter J. Wheatley 《Monthly notices of the Royal Astronomical Society》1998,301(1):95-100

We present low–medium resolution optical spectroscopy of the eclipsing AM Her system MN Hya (RX J0929–24). We determine the magnetic field strength at the primary accretion region of the white dwarf to be 42 MG from the spacing of cyclotron features visible during π ∼ 0.4–0.7. From spectra taken during the eclipse we find that the secondary has an M3–4 spectral type. Combined with the eclipse photometry of Sekiguchi, Nakada &38; Bassett and an estimate of the interstellar extinction we find a distance of ∼300–700 pc. We find unusual line variations at π ∼ 0.9: Hα is seen in absorption and emission. This is at the same point in the orbital phase at which a prominent absorption dip is seen in soft X-rays.  相似文献   

PSR J1012+5307: younger than it looks?     

L. Burderi  A. R. King  & G. A. Wynn 《Monthly notices of the Royal Astronomical Society》1998,300(4):1127-1130

Lorimer et al. have recently reported that the spin-down age (∼7 × 10⁹ yr) of the low-mass binary pulsar PSR J1012+5307 is much higher than the cooling age (3 × 10⁸ yr) of its white dwarf companion. The proposed solutions for this discrepancy are outlined and discussed. In particular, the revised cooling age estimate proposed by Alberts et al. agrees with data from other low-mass binary pulsar systems if a transition to the 'classical' cooling regime occurs between ∼0.14 and ∼0.28 M_⊙. If this transition is excluded, PSR J1012+5307 seems to have finished its accretion phase far from the spin-up line.  相似文献   

Study on the fractal character of magnetic anomaly fields and the delineation of tectonic elements in the South China Sea     

姜效典  于增慧 《中国海洋湖沼学报》1998,16(1):28-35

INTRODUCTION~hon0ffornjcelmtSwnthebasisofthestudyonthecrustaldefonnationanddeVel0prnent,thedistributionofndnereIs,andthendnerogeneticlawr.ThegeornagneticfieklisthecomP0siterefledionoftheformati0nanddefortnationofthecrust.Sornagnct-icsLLrVeydatacomPriseirnPortantbasisfordelincatingthearchiteCtonicelements,dCtendningtheirboundarylines,andanalopngthesanndarystrudriineachelernent,whicharetthernaintasks0fgoophySicalworkers.Thegoornagneticdelineati0nofanareahadforlongbodonequalitativeybyobs…  相似文献   

Measurements of the direction of the solar wind using interplanetary scintillation     

P. J. Moran  A. R. Breen  C. A. Varley  P. J. S. Williams  W. P. Wilkinson  J. Markkanen 《Annales Geophysicae》1998,16(10):1259-1264

EISCAT observations of the interplanetary scintillation of a single source were made over an extended period of time, during which the orientation of the baselines between the two observing sites changed significantly. Assuming that maximum correlation between the scintillations observed at the two sites occurs when the projected baseline is parallel to the direction of plasma flow, this technique can be used to make a unique determination of the direction of the solar wind. In the past it has usually been assumed that the plasma flow is radial, but measurements of eleven sources using this technique have indicated conclusively that in at least six cases observed at mid or high heliocentric latitude there is a significant non-radial component directed in four cases towards the heliocentric equator and in two cases towards the pole.  相似文献