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991.
建立了一个试验用地名库和地理语料库,在此基础上构建对地名用字可信度的统计分析模型。通过分析地名在中文文档中的使用习惯和规律,总结出经常与地名一起使用的且具有地名指示含义的辅助字或词,以此为基础建立地名识别辅助词词库和地名识别的规则库。对地名库和地理语料库的用字进行统计分析,通过设定地名用字可信度概率阈值和辅助词指示作用对文本中潜在地名进行初步的筛选形成候选地名;在粗筛选产生的候选地名基础上结合地名识别规则进一步确认,以提高地名识别的准确率。  相似文献   
992.
红运水源地地处嘉祥断块北部,主要含水层为奥陶纪三山子组中细晶白云岩,且岩溶发育,在岩性上中细晶白云岩细晶白云岩泥灰岩灰岩和豹皮灰岩微晶白云岩。区域断裂构造发育,多以张性断裂为主,一般为带状岩溶发育,深度143~330m,与断裂构造的走向基本一致,为地下水的富存和运移提供了良好的场所和通道。奥陶系顶板不同埋藏深度形成的高差,为岩溶地下水径流提供了强烈的地下水动力条件。通过研究岩溶发育特征,对比区域地质、水文地质条件,证实岩溶发育与地层岩性、地质构造、地下水动力条件、埋藏深度等关系密切。通过对比钻孔地层资料,分析了红运水源地富水性条件,地层岩性是岩溶发育的物质基础,地质构造是岩溶发育的控制因素,水动力条件是岩溶发育的外在因素,对指导北方覆盖型岩溶地下水勘查及寻找覆盖型岩溶水富集区具有借鉴意义。  相似文献   
993.
层序地层研究表明,位于扬子地块西南缘的黔西南地区在中三叠世末期(相当于Ladinian-Carnian期)出现了一次与全球同步的大规模海侵,形成了一个向上变深的碳酸盐岩台地淹没沉积层序。垄头组顶部和竹竿坡组分别是海进体系域(TST)的下、上部分。碳、氧同位素研究表明,垄头组顶部自下而上δ(18O)持续增大,而δ(13C)先逐渐增大,后在顶部界面附近快速下降,反映了垄头组顶部在暴露环境下氧化作用的结果。竹竿坡组δ(13C)自下而上逐渐增大,δ(18O)总体呈现逐渐减小趋势,反映了海平面变化特征。研究认为,海进体系域的δ(13C)和δ(18O)演化不但反映了海平面和沉积环境变化,同时对密集段(CS)、层序界面和古暴露面等也有很好的识别作用,在层序地层研究中具有重要的意义。  相似文献   
994.
?????????г???????????????????????????????????????????????????????????????????????????α?????????黯???α?????????????????????????????????α?????????????????????????????????????е????????????,??????????α???????????  相似文献   
995.
为了研究青海省鄂拉山地区找矿远景,基于该区最新一轮1∶5万水系沉积物测量数据,提炼分析其地球化学特征之元素分布特征、元素组合特征、元素异常特征,认为该区主要成矿元素为W,Sn,Mo,Bi,Ag,Cu,Pb,Zn,Au,Sb;并指出该类成矿元素多在元古宙和古生代的地层中明显富集;主要成矿类型为矽卡岩型和热液充填型。结合已知成矿地质条件,最终优选出4个找矿远景区,为该区域提供了较明确的找矿方向。  相似文献   
996.
蒙阴盆地是在库拉板块向亚洲大陆下俯冲,中国东部隆升伸展板块裂解阶段发育起来的。在中生代,盆地的成生演化经历了侏罗纪拗陷盆地发育阶段和早白垩世拗陷—裂陷阶段。在相应沉积演化过程中,形成侏罗纪湖相红色碎屑岩建造,早白垩世早期滨浅湖—半深湖相灰绿色细粒陆屑岩沉积,早白垩世中期河湖相凝灰质复陆屑岩类夹火山碎屑岩类沉积,早白垩世晚期中基性火山熔岩、火山碎屑岩组合。沉积中心在侏罗纪和早白墨世早期皆偏于西北部,此后,向东南部迁移。晚白垩世,盆地处于风化剥蚀阶段。古近纪,受新生太平洋板块向亚洲大陆下俯冲影响,盆地又处于拗陷—裂陷阶段,相应形成山间河湖相—山麓堆积相类磨拉石建造。古近纪末期,该盆地整体隆起处于长期风化剥蚀状态。  相似文献   
997.
A two‐dimensional (2D) finite‐difference shallow water model based on a second‐order hybrid type of total variation diminishing (TVD) approximate solver with a MUSCL limiter function was developed to model flooding and inundation problems where the evolution of the drying and wetting interface is numerically challenging. Both a minimum positive depth (MPD) scheme and a non‐MPD scheme were employed to handle the advancement of drying and wetting fronts. We used several model problems to verify the model, including a dam break in a slope channel, a dam break flooding over a triangular obstacle, an idealized circular dam‐break, and a tide flow over a mound. Computed results agreed well with the experiment data and other numerical results available. The model was then applied to simulate the dam breaking and flooding of Hsindien Creek, Taiwan, with the detailed river basin topography. Computed flooding scenarios show reasonable flow characteristics. Though the average speed of flooding is 6–7 m s?1, which corresponds to the subcritical flow condition (Fr < 1), the local maximum speed of flooding is 14·12 m s?1, which corresponds to the supercritical flow condition (Fr ≈ 1·31). It is necessary to conduct some kind of comparison of the numerical results with measurements/experiments in further studies. Nevertheless, the model exhibits its capability to capture the essential features of dam‐break flows with drying and wetting fronts. It also exhibits the potential to provide the basis for computationally efficient flood routing and warning information. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   
998.
Wang  ZhenQi  Zhi  DongMing  Zhang  ChangMin  Xue  XinKe  Zhang  ShangFeng  Li  TianMing  Yang  Fei  Liu  LouJun  Cheng  Liang  Lu  Dong  Zhou  FengJuan  Chen  YuanYong 《中国科学:地球科学(英文版)》2010,52(1):106-114

Well che89, located in the Chepaizi area in the northwest margin of Junggar basin, acquires high production industrial oil flow, which is an important breakthrough in the exploration of the south foreland slope area of Junggar basin. The Chepaizi area is near two hydrocarbon generation depressions of Sikeshu and Shawan, which have sets of hydrocarbon source rock of Carboniferous to Jurassic as well as Upper Tertiary. Geological and geochemical parameters are proper for the accumulation of mixed source crude oil. Carbon isotope, group composition and biomarkers of crude oil in Upper Tertiary of well Che89 show that the features of crude oil in Upper Tertiary Shawan Formation are between that of Permian and Jurassic, some of them are similar to these two, and some are of difference, they should be the mixed source of Permian and Jurassic. Geochemical analysis and geological study show that sand extract of Lower Tertiary Wulunguhe Formation has the same source as the crude oil and sand extract of Upper Tertiary Shawan Formation, but they are not charged in the same period. Oil/gas of Wulunguhe Formation is charged before Upper Tertiary sedimentation, and suffered serious biodegradation and oxidation and rinsing, which provide a proof in another aspect that the crude oil of Upper Tertiary Shawan Formation of well Che89 is not from hydrocarbon source rock of Lower Tertiary.

  相似文献   
999.
This study focuses on the three‐dimensional (3‐D) characteristics of wave propagation in pipe‐pile using elastodynamic finite integration technique. First, a real 3‐D pile‐soil model in cylindrical coordinate system is presented. Then, the governing equations are established. With the boundary and initial conditions, the numerical solution is obtained. The accuracy and feasibility of the self‐written code are further verified via comparing with the measured data. Velocity histories at different angles of pile top and pile tip are illustrated, and the snapshots reflecting the 3‐D characteristics of wave propagation are given. It shows that the interferences of Rayleigh waves can confuse the result interpretation for pile integrity testing. The increase of hammer contact time can effectively mitigate the interferences, and the interferences of Rayleigh waves are weakest at an angle of 90° from where hammer hits. Besides, surrounding soil can partly mitigate the wave interferences. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   
1000.
Theoretical electron density sensitive line ratios   R 1– R 6  of Si  x soft X-ray emission lines are presented. We found that these line ratios are sensitive to electron density n e, and the ratio R 1 is insensitive to electron temperature T e. For reliable determination of the electron density of laboratory and astrophysical plasmas, atomic data, such as electron impact excitation rates, are very important. Our results reveal that the discrepancy of the line ratios from different atomic data calculated with the distorted wave (DW) approximation and the R-matrix method is up to 19 per cent at   n e= 2 × 108 cm−3  . We applied the theoretical intensity ratio R 1 to the Low Energy Transmission Grating Spectrometer (LETGS) spectrum of the solar-like star Procyon. By comparing the observed value (1.29) with the theoretical calculation, the derived electron density n e is  2.6 × 108 cm−3  , which is consistent with that derived from  (C  v < 8.3 × 108 cm−3)  . When the temperature structure of the Procyon corona is taken into account, the derived electron density increases from   n e= 2.6 × 108  to  2.8 × 108 cm−3  .  相似文献   
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