共查询到20条相似文献，搜索用时 859 毫秒
1.
藏北高原地区干、雨季大气边界层结构的不同特征 总被引：6，自引：2，他引：4
利用2004年4月预试验期(PIOP)和8月加强期(IOP)的无线电探空仪观测资料,分析了藏北高原地区干、雨季大气边界层结构的不同特征.结果显示:藏北高原地区边界层虚位温、比湿等日变化大,对流混合层高度较高,高度干季在2 211～4 430 m之间,雨季在1 006～2 212 m之间,干季的对流混合层高度明显高于雨季... 相似文献
2.
藏北高原夏季典型天气大气边界层特征分析 总被引：7，自引：0，他引：7
利用加密探空资料,分析了藏北高原那曲和安多地区夏季典型晴天与阴天边界层风速、位温与比湿时空分布及变化特征.结果发现:在夏季8月,上述地区东西分量风速(切变)晴天均比阴天小,安多地区盛行偏西风,那曲地区盛行偏东风;南北分量风速(切变)晴天比阴天大.边界层晴天和阴天白天(晚上)的对流(稳定)边界层特征明显,阴天稳定边界层的厚度和对流边界层的高度较晴天时的都低;比湿夜间比白天大,阴天比晴天大.在安多地区和那曲地区都出现了逆湿现象,强逆湿主要出现在午夜或正午. 相似文献
3.
河套干旱地区夏季边界层结构特征观测分析 总被引：2，自引：0，他引：2
利用2013年夏季7月爱尔达K/LLX802J型机动式边界层风廓线雷达获取的三维风场资料和银川站高空气象探测资料,对河套干旱地区夏季边界层日变化特征进行了分析.结果表明:爱尔达K/LLX802J型机动式风廓线雷达能较好的反映并分辨出夏季河套干旱地区边界层内大气湍流和风场的演变过程.夏季7月河套干旱地区边界层高度白天平均为2127.2 m,夜间平均为1760.7 m,白天边界层高度比夜间平均高366.5 m.河套干旱区夏季地表非绝热加热对边界层的影响主要集中在800 m以下,800~2000 m高度边界层则主要受昼夜交替和大尺度天气系统的影响.夏季7月河套干旱地区边界层风速在300 m以下随高度增加而增大,离地500 m以下边界层易在北京时间07:00-11:00和18:00-21:00时段发生风速切变;300 m以下边界层白天盛行西南偏南风、夜间盛行南风,300~2000 m高度边界层白天和夜间均盛行东南风;离地300 m以下边界层易在夜间21:00-23:00时出现风向切变.夏季7月白天河套干旱地区边界层大气垂直速度在300 m高度以下随高度增加而增大,由0.3 m·s-1增大到0.6 m·s-1,夜间边界层大气垂直速度在200 m高度以下随高度增大而增大;300 m高度以上边界层大气垂直速度无论昼夜随高度变化均较小. 相似文献
4.
珠峰地区夏季大气边界层结构初步分析 总被引：6，自引：2，他引：4
利用中国科学院珠穆朗玛峰大气与环境综合观测研究站2007年7、 8月的部分无线电探空资料和风温廓线仪资料, 分析了珠峰地区夏季大气边界层结构. 结果表明: 珠峰地区夏季边界层高度日变化较大, 气温日变化明显. 下午和傍晚可能因为冰川风的存在, 多为偏南风, 风力相对较大. 珠峰地区风速时空变化较大, 特别是下午, 在上空大约1 800 m到2 300 m处风速多为随高度增大, 再往上又减小, 而且此处多为偏西风和偏东风. 这可能与大尺度的大气环流有关, 受地形和冰川影响相对小得多. 相似文献
5.
藏北高原土壤温湿变化特征分析 总被引：12，自引：2，他引：10
利用"全球协调加强观测计划(CEOP)亚澳季风之青藏高原试验"(CAMP/Tibet,2001—2010)的观测资料,从不同的时间尺度分析了藏北高原不同地点不同深度的土壤温度和土壤湿度变化特征.结果表明:10 cm以上日平均土壤温度呈正弦变化,而10 cm以下土壤温度变化不大;各层土壤温度最高都出现在7～8月;年际气候的差异至少可以反映到40 cm土壤;各层土壤湿度无明显日变化,存在明显月变化,夏季降水量的多少对各层土壤湿度都有明显的影响. 相似文献
6.
藏北高原多年冻土区地表反照率特征分析 总被引：9，自引：5，他引：4
利用青藏高原冰冻圈观测研究站西大滩、五道梁和唐古拉自动气象站(AWS)2006—2007年的辐射观测资料,分析了藏北高原多年冻土区不同下垫面的地表反照率特征.结果表明:该地区地表反照率在四季都表现出明显的日变化特征,呈U形,早晚大,中午小.日平均和月平均地表反照率有相同的年变化特征,且冬半年的地表反照率远远大于夏半年.受积雪的影响,地表反照率年均值较高,夏季最小,冬季最大,春季大于秋季.针对3种不同植被类型的下垫面,在四季反照率都有高寒草甸(唐古拉)高寒草原(西大滩)荒漠草原(五道梁)的特点. 相似文献
7.
8.
极端干旱荒漠区典型晴天大气热力边界层结构分析 总被引：3，自引：1，他引：3
利用极端干旱区敦煌野外观测试验资料，分析了极端干旱荒漠区夏季典型晴天位温、风速、比湿等主要物理要素的垂直结构特征及其地表热力和近地层大气运动特征的日变化规律。发现在极端干旱地区夏季晴天大气热力边界层结构十分独特。在夜间，贴地逆温层最低在900 m以上，最厚可以达到1 750 m，逆温层上面的残余层一般能达到4 000 m左右的高度。在白天，位温超绝热递减层高达1 000 m，超绝热递减层上面的混合层最高达3 700 m，混合层顶上还有大约450 m甚至更厚的夹卷层。当白天对流层发展达到残余层以后，混合层的发展明显加快。风速和比湿垂直廓线特征很好地印证了大气热力边界层独特的结构特征，地表热力和近地层大气运动特征也为这种独特的大气热力边界层结构提供了较好的物理支持。 相似文献
9.
新疆夏季变湿的大气环流异常特征 总被引：14，自引：3，他引：11
利用1961-2003年NCEP/NCAR再分析资料和中国气象局整编的新疆夏季(6~8月)月降水量资料,分析了新疆夏季1971-1986年干旱期和1987-2003年湿润期的大气环流变化异常特征.结果表明:在平均环流场上,中亚-巴尔喀什湖槽及上下游地区脊的增强是新疆地区夏季变湿的环流场特征之一,且中亚-巴尔喀什湖槽随高度增加强度明显增强,200 hPa达到最强;源于低纬阿拉伯海向北直至中亚对流层低层偏南的强气流是湿润期环流异常、降水增多的又一特征,也是水汽重要来源之一;中亚上空高空急流轴南压是新疆夏季湿润期与干旱期高空急流最重要的差异特征. 相似文献
10.
《地球科学进展》2020,(5)
黑潮延伸体海区是冬季西北太平洋向大气加热的关键海区。前人研究表明活跃在黑潮延伸体海区的海洋涡旋会通过影响海表面温度而影响海面风。回顾了最近几年该海域海洋涡旋影响局地大气的研究成果,重点从船测探空资料、卫星观测资料和模式数值实验3个方面分析和比对了已有的研究成果,依据该海区海洋涡旋导致大气异常的地转适应理论,得到了如下新的科学推论:海洋涡旋上空大气运动较慢时,大气对海洋涡旋的响应表现以气压调整机制为主,海洋涡旋的影响常常被限制在大气边界层中;海洋涡旋上空大气的运动较快时,大气对暖(冷)涡的响应以垂直混合机制为主,海表面风速在暖(冷)水上加(减)速,海表面风强辐合出现在暖水的背景风下游一侧,并从暖水上空携带了大量水汽;通过水汽凝结与海面辐合上升之间的正反馈机制,为导致大气中出现强对流提供了必要条件。该推论将有利于进一步定量刻画海洋涡旋对大气的影响。 相似文献
11.
Guboglo M. N. 《GeoJournal》1980,4(1):53-58
International unity is becoming ever stronger in this country owing to an increasing similarity in the development of the cultural environment. This comprises the provision of all the country's republics with a sufficient number of schools, theatres, and other institutions and cultural information media in accordance with the needs of the population. An important part is played by the rise in ‘the general educational level, as well as the level of professional qualifications and skills. Among all the Soviet nations and nationalities, this rise being more rapid among formerly backward peoples. Prominent among the factors of internationalization is the progressive development of the nationalities’ cultural resources, while professional culture is being increasingly brought within the reach of the masses.The implementation of the nationalities policy promotes the all-round development of all Soviet nations and nationalities, their drawing together, the upsurge of the individual capabilities of every Soviet citizen. 相似文献
12.
Deviation of the major axis of the inertia ellipsoid of the Moon from the direction toward the Earth
B. P. Kondratyev 《Astronomy Reports》2017,61(8):709-714
It is known from observations that the center of mass of the Moon does not coincide with the geometric center of its figure, and the line connecting these two centers is not aligned with the direction toward the center of the Earth, instead deviating toward the Southeast. This stationary deviation of the axis of the inertia ellipsoid of the Moon to the South of the direction toward the Earth is analyzed. A system of five linear differential equations describing the physical libration of the Moon in latitude is considered, and these equations are derived using a new vector method taking into account perturbations from the Earth and partly from the Sun. The characteristic equation of this system is obtained, and all five oscillation frequencies are found. Special attention is paid to the fifth (zero) frequency, for which the solution of the latitude libration equations are stationary and represents a previously unknown additional motion of the rotational axis of theMoon in a cone with a small opening angle. In contrast to the astronomical precession of the Earth, the rotation of the angular-velocity vector is in the positive direction (counter-clockwise), with the period T 3 = 27.32 days. On this basis, this phenomenon has been named “quasi-precession.” This quasi-precession leads to a stationary inclination of the major axis of the inertia ellipsoid of theMoon to the South (for an observer on Earth), making it possible to explain one component of the observed deviation of the center of mass of the Moon from the direction toward the Earth. The opening angle of the quasiprecession cone is approximately 0.834″. 相似文献
13.
14.
Chronological analyses of correlations between certain global repeating events (mass extinctions of marine organisms, meteorite impacts, and flashes in the frequency of geomagnetic reversals) during the Phanerozoic Eon and the motion of the solar system in the Galaxy are presented for five rotationally symmetrical models for the regular Galactic gravitational field. Thirteen of sixteen mass-extinction events can be described by a repetition interval of 183±3 million years. This is in agreement with the anomalistic period (interval between two subsequent passages of the Sun through the apocenter of its Galactic orbit) in the model of Allen and Martos. The positions of the minima and maxima in Gaussian functions approximating the frequency distribution for geomagnetic reversals also agree with the times of passage of the Sun through the apocenter and pericenter, respectively, of its Galactic orbit in this model. The maximum in the distribution of the deviations of the dates of mass extinctions from the nearest dates of impacts of large, crater-forming bodies is close to zero, providing evidence that many such events are correlated. As a rule, extinctions follow impact events. The impacts of large bodies have occurred most often when the solar system passes through the Galactic plane, while mass extinctions occur more often at some distance from the Galactic plane (about 40 pc). As a rule, intervals of increases in the frequency of geomagnetic reversals coincide with dates of impacts of large bodies. At the same time, these intervals do not show a clear correlation with the dates of mass extinctions. The intensity of mass extinctions, like the energy released by impacts, is consistently higher in periods when the Sun is moving from the apocenter toward the pericenter of its orbit, than when it is moving from the pericenter toward the apocenter. Thus, there is evidence for a variety of relationships between repeating global events in the Phanerozoic and the motion of the Sun in the Galaxy. Long-period variations in the frequency of geomagnetic reversals are correlated with the orbital motion of the Sun, and increases in the frequency of geomagnetic reversals are correlated with impacts. Mass extinctions are correlated with the impacts of large bodies, whose motions may have been perturbed by clouds of interstellar material concentrated toward the Galactic plane and by the shock front associated with the Perseus spiral arm, through which the solar system passes. The velocity of the Sun relative to the spiral pattern is estimated. 相似文献
15.
位于华北和扬子两板块碰撞带中的苏鲁榴辉岩形成的温压条件不但是超高压，而且是高温。榴辉岩的PTt轨迹表明其为陆-陆磁撞俯冲带的产物。榴辉岩的区域性围岩花岗质片麻岩为新元古代同碰撞期花岗岩，榴辉岩及其他直接围岩皆呈包体存在于其中，并见新元古代花岗岩呈脉状侵入榴辉岩包体中。区域性围岩新元古代花岗岩的锆石中发现有柯石英、绿辉石等包裹体，表明新元古代花岗岩的组成物质也经受过超高压变质作用，且榴辉岩与围岩新元古代花岗岩的锆石U-Pb体系同位素年龄基本相同。但新元古代花岗岩所记录的变质作用和变形作用期次（或阶段）却少于榴辉岩。椐上述可得如下推断：超高压榴辉岩与新元古代花岗岩岩浆是同时在碰撞带底部（俯冲板块前部）形成的；榴辉岩的第一折返阶段是由新元古代花岗岩岩浆携带上升的，其第二折返阶段是和新元古代花岗岩一起由逆冲及区域性隆起而上升，遭受剥蚀。 相似文献
16.
某高速公路下伏煤矿采空区稳定性分析 总被引：10，自引：0，他引：10
在论述某高速公路下伏砦脖煤矿采空区地质、采矿和工程地质特征的基础上, 进行了稳定性数值模拟分析, 定性与定量地分析与评价了该煤矿采空区的地表变形特征及稳定性。研究结果表明: 该煤矿采空区的变形尚未完成, 对拟建的高速公路将产生很大的危害, 必须采取相应的工程治理措施。 相似文献
17.
18.
摩擦桩基桩土间极限摩阻力取值问题探讨 总被引：1，自引：0，他引：1
通过对广珠东线高速公路横沥大桥的试桩及土体的工程地质条件分析,总结出影响摩擦桩基桩土间极限摩阻力取值的一般问题以及解决问题的方法和措施。 相似文献
19.
The Importance of the Precipitation and the Susceptibility of the Slopes for the Triggering of Landslides Along the Roads 总被引：3，自引：1，他引：2
Clemente Irigaray Francisco Lamas Rachid El Hamdouni Tomás Fernández José Chacón 《Natural Hazards》2000,21(1):65-81
In order to characterise the influence of the heavyrains on the observed landslides during the 1996–1997hydrological cycle, rainfall records for the last 100years are analysed from 104 stations in easternAndalusia. Regarding the amounts of rain recordedbetween October 1996 and March 1997 in the 104stations studied, 31 presented new all-time records;15 presented values that were 80–100% of thepre-1995 record; 49 stations, 80–50%; and 9stations, < 50%. A map has been devised of thesusceptibility of the materials through which thesouth-eastern Andalusian road network crosses,together with an inventory of the damage caused byinstability phenomena on banks and cuttings of theroad network during the winter of 1996–1997. Therelationships between the rainfall during the studyperiod, the damage caused to the road network and thesusceptibility of the materials affected are analysed.The results indicate that there is a clearcorrespondence between the rainfall recorded and thesusceptibility of the materials with the inventorieddamage. It is concluded that the widespread seriousdamage caused in early 1997 to the roads andsurrounding areas in the Alpujarra region and thecoast of the Province of Granada was mainly caused bythe extraordinarily heavy rains. However, considerablyless damage was observed where the susceptibility ofthe terrain is low, thus highlighting the extremeusefulness of terrain-susceptibility maps for riskprevention and territorial planning. 相似文献
20.
The structure of the eastern Pyrenees consists mainly of south-directed thrusts involving basement and cover rocks. An antiformal stack developed by the piling up of basement thrust sheets which outcrop in the Axial zone. These structures account for a thin-skinned thrust model rather than a vertical fault model in which the Axial zone would be essentially autochthonous, and the North-Pyrenean fault the axial plane of a fan thrust system. New data from the Eastern Pyrenees and the thin-skinned model suggest that(1) the structure east of the Pedraforca nappe is similar to that of the Central Pyrenees; (2) the cover rocks of the South-Pyrenean units and of the Axial zone-after restoration—built up a northwards-thickening prism consistent with the existence of a unique Pyrenean sedimentary basin during Mesozoic time; (3) the Axial zone is only a complex antiformal stack developed as a part of South-Pyrenean system related to the Paleogene thrusting-tectonics. The Axial zone palaeogeographic area had no special meaning during Mesozoic time. 相似文献