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31.
Laboratory experiments on the impact disruption of ice-silicate mixtures were conducted to clarify the accretion process of small icy bodies. Since the icy bodies are composed of ice and silicates with various porosities, we investigated the effect of porosity on the impact disruption of mixtures. We tested the mixture target with the mass ratio of ice to silicate, 0.5 and with 5 different porosities (0, 12.5, 25, 32, 37%) at the impact velocities of 150 to 670 m/s. The silicate mass ratio was changed from 0 to 0.5 in steps of 0.1 at a porosity of 12.5% and a constant impact velocity of about 300 m/s. The impact strength of the mixture was found to decrease with increasing porosity and the silicate mass ratio between 0.1 and 0.5 could enhance the strength of the icy target. The observed dependence of the impact strength on the porosity is opposite to that observed for pure ice. This difference could play an important role in ice-silicate fractionation during the accretion process. Because, ice rich bodies are easily broken as the porosity decreases in their evolution, the collisional growth could be prohibited. On the other hand, among the silicate rich bodies the collisional growth could be enhanced.  相似文献   
32.
河南省春季气候变化及其对小麦产量构成要素的影响   总被引:4,自引:0,他引:4  
目前有关气候变化及其对农作物产量影响的研究较多,而对产量构成要素的影响研究相对较少。本文利用自然正交函数(EOF)分解、相关分析、趋势倾向率分析等方法对河南省近30多年的气候和近20多年的小麦产量构成三要素———穗数、粒数、粒重进行了时空变化特征分析,在此基础上分析了春季气候变化对小麦产量及其构成要素的影响。结果表明:全省春季平均气温、降水量、日照时数变化具有比较好的空间一致性,平均气温呈比较明显的上升趋势,降水呈不太明显的下降趋势,日照呈一定的下降趋势;小麦粒重和产量变化具有较好的空间一致性,而穗数、粒数则具有反位相空间变化特征,穗数、粒重及产量均呈明显的上升趋势,粒数呈抛物线变化趋势,其中1991年后呈明显上升趋势;平均气温的升温变化趋势有利于小麦粒重、穗数和最终产量的提高,但不利于粒数增加;降水变化趋势不利于粒重提高,对其他产量构成要素影响不明显;日照的变化对产量及各构成要素影响不明显。  相似文献   
33.
根据1971~2010年民勤近40a气象资料、民勤周边县市沙尘暴资料,详细分析了民勤绿洲沙尘暴变化特征及影响因素,结果表明:①绿洲以局地性沙尘暴为主,但区域性沙尘暴无论是持续时间、伴随的大风强度和成灾性均大于局地性沙尘暴。②一日中局地性和区域性沙尘暴主要出现在下午和傍晚;月际变化除3月份外其它月份局地性均较区域性沙尘暴多,6~8月份偏多明显,各季局地性均比区域性沙尘暴多,夏季偏多明显;年际局地和区域性沙尘暴均为显著减少趋势,年代际为明显减少趋势。③干旱气候、丰富的沙源是民勤多沙尘暴的自然原因,气候的变化和下垫面状况的改善使沙尘暴减少。分析表明气候变暖使大风日数减少、风力减小,从而影响局地和区域性沙尘暴减少,气候变暖使日照时数增长、蒸发增大,从而影响区域性沙尘暴减少,而对局地性沙尘暴的减少影响不大。  相似文献   
34.
黄河上游流域蒸散量及其影响因子研究   总被引:38,自引:0,他引:38  
利用彭曼公式计算了80年代以来黄河上游流域蒸散量,分析了该地区蒸散量、日照时数、气温、空气饱和差等气候因子的变化趋势,着重研究了诸因子对蒸散量的影响。研究发现,黄河上游流域蒸散量呈逐年增大趋势,并以每年3.25 mm的速度递增;而作为主要影响因子的日照时数则以每年3.6小时的速度增加;气温同样表现出逐年升高的趋势,其气候倾向率为0.4℃/10 a;空气饱和差也以每年0.02 hPa的速度递增。因此,可以认为,黄河上游流域日照时数、气温及饱和差的增加,加剧了草地蒸散量的增大,而蒸散量的增大和降水量的减少则直接影响到了黄河上游流量的减少和草地荒漠化的蔓延。  相似文献   
35.
I.D.S. Grey 《Icarus》2004,168(2):467-474
Research on the impact cratering process on icy bodies has been largely based on the most abundant ice, water. However little is known about the influence of other relatively abundant ices such as ammonia. Accordingly, data are presented studying the influence on cratering in ammonia rich ice using spherical 1 mm diameter stainless steel projectiles at velocities of 4.8±0.5 km s−1. The ice target composition ranged from pure water ice, to solutions containing 50% ammonia and 50% water by weight. Results for crater depth, diameter, volume and depth/diameter ratio are given. The results showed that the presence of ammonia in the ice had a very strong influence on crater diameter and morphology. It was found that with only a 10% concentration of ammonia, crater diameter significantly decreased, and then at greater concentrations became independent of ammonia content. Crater depth was independent of the presence of ammonia in the ice, and the crater volume appeared to decrease as ammonia concentration increased. Between ammonia concentrations of 10 and 20% crater morphology visibly changed from wide shallow craters with a deeper central pit to craters with a smoothly increasing depth from the crater rim to centre. Thus, a small amount of ammonia within a water ice surface may have a major effect on crater morphology.  相似文献   
36.
电影不仅是作为一种艺术品,同时也是作为一种商品存在,而电影片名就好比是电影的一件外衣,因此,确切地翻译电影片名非常重要。电影片名的翻译技巧有很多,同时影响电影片名的翻译的因素也有很多。因此,在翻译电影片名时要从各方面因素考虑,从而选择恰当的翻译技巧,使得译名不仅能够从意义上忠实于源名,涵盖电影的内容,同时在形式上做到简练并具有吸引力。  相似文献   
37.
All of the large impact features of the middle-sized icy satellites of Saturn and Uranus that were clearly observed by the Voyager spacecraft are described. New image mosaics and stereo-and-photoclinometrically-derived digital elevation models are presented. Landforms related to large impact features, such as secondary craters and possible antipodal effects are examined and evaluated. Of the large impacts, Odysseus on Tethys appears to have had the most profound effect on its “target” satellite of any of the impact features we examined. Our modeling suggests that the Odysseus impact may have caused the prompt formation of Ithaca Chasma, a belt of tectonic troughs that roughly follow a great circle normal to the center of Odysseus, although other hypotheses remain viable. We identify probable secondary cratering from Tirawa on Rhea. We attribute a number of converging coalescing crater chains on Rhea to a putative, possibly relatively fresh, ∼350 km-diameter impact feature. We examine the antipodes of Odysseus, the putative ∼350 km-diameter Rhean impact feature, and Tirawa, and conclude that evidence from Voyager data for damage from seismic focusing is equivocal, although our modeling results indicate that such damage may have occurred. We propose a number of observations and tests for Cassini that offer the opportunity to differentiate among the various explanations and speculations reviewed and evaluated in this study.  相似文献   
38.
本文通过历史与现代过程的分析,探讨了历史上治黄治淮的环境效应,特别是黄河筑堤和淮河高家堰修筑所造成的环境后果。黄河筑堤为下游平原地区的开发提供了条件,但河床的抬高,地上河的形成,使黄河改道频繁,并由此控制了徽地貌的形成,影响了土壤的成土过程和分布、地表水和地下水动念、涝渍灾害和盐碱化。黄河夺淮后,高家堰的修筑使洪泽湖面积急剧扩大,水位迅速提高,并使之成为中国和世界上最早的大水库。并由此增加了洪涝灾害的机遇和频率。  相似文献   
39.
CSDP core Yaxcopoil-1 was drilled to a depth of 1,511 m within the Chicxulub crater. An organic-rich marly limestone near the base of the hole (1,495 to 1,452 m) was deposited in an open marine shelf environment during the latest Cenomanian (uppermost Rotalipora cushmani zone). The overlying sequence of limestones, dolomites and anhydrites (1,495 to 894 m) indicates deposition in various carbonate platform environments (e.g., sabkhas, lagoons). A 100-m-thick suevite breccia (894–794 m) identifies the Chicxulub impact event. Above the suevite breccia is a dolomitic limestone with planktic foraminiferal assemblages indicative of Plummerita hantkeninoides zone CF1, which spans the last 300 ky of the Maastrichtian. An erosional surface 50 cm above the breccia/dolomite contact marks the K/T boundary and a hiatus. Limestones above this contact contain the first Tertiary planktic foraminifera indicative of an upper P. eugubina zone P1a(2) age. Another hiatus 7 cm upsection separates zone P1a(2) and hemipelagic limestones of planktic foraminiferal Zone P1c. Planktic foraminiferal assemblages of Zone Plc to P3b age are present from a depth of 794.04 up to 775 m. The Cretaceous carbonate sequence appears to be autochthonous, with a stratigraphic sequence comparable to late Cretaceous sediments known from outside the Chicxulub crater in northern and southern Yucatan, including the late Cenomanian organic-rich marly limestone. There is no evidence that these sediments represent crater infill due to megablocks sliding into the crater, such as major disruption of sediments, chaotic changes in lithology, overturned or deep dipping megablocks, major mechanical fragmentation, shock or thermal alteration, or ductile deformation. Breccia units that are intercalated in the carbonate platform sequence are intraformational in origin (e.g., dissolution of evaporites) and dykes are rare. Major disturbances of strata by the impact therefore appear to have been confined to within less than 60 km from the proposed impact center. Yaxcopoil-1 may be located outside the collapsed transient crater cavity, either on the upper end of an elevated and tilted horst of the terrace zone, or even outside the annular crater cavity. The Chicxulub site thus records a large impact that predates the K/T boundary impact and mass extinction.  相似文献   
40.
Recently, multi-layered targets have become commonplace in both military and civilian applications, such as marine hulls, armored vehicle bodies, outside structures of bulletproof cars, and aerospace vessels. This paper studies the resistant performance of perforation in multi-layered targets. An estimation procedure is established based on the concepts of the conservation of momentum, impulse-momentum law, and conservation of energy. Experimental results of the test of Almohandes et al. are adopted to check the residual velocity of multi-layered targets. The results of the verification are good in terms of agreement for impact velocities ranging from 700 to 800 m/s, when the ratio of the projectile length to the projectile diameter (i.e. L/D) is 4.2, and the average residual velocity error of single, double- or triple-layered targets range approximately from 4.42 to 8.40%. The ballistic performance is best for the double target when the ratio of the first layer thickness to the total thickness (i.e. t1/(t1+t2)) is about 0.75, and the worse performance occurs when the ratio t1/(t1+t2) is 0.5. An air gap slightly influences the resistant performance of perforation in multi-layered targets. These results may serve as a useful reference for designers.  相似文献   
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