首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   71232篇
  免费   1127篇
  国内免费   659篇
测绘学   1714篇
大气科学   5030篇
地球物理   14214篇
地质学   25229篇
海洋学   6164篇
天文学   16332篇
综合类   208篇
自然地理   4127篇
  2022年   397篇
  2021年   704篇
  2020年   778篇
  2019年   825篇
  2018年   1893篇
  2017年   1759篇
  2016年   2235篇
  2015年   1318篇
  2014年   2176篇
  2013年   3766篇
  2012年   2276篇
  2011年   3118篇
  2010年   2605篇
  2009年   3504篇
  2008年   3255篇
  2007年   3045篇
  2006年   2876篇
  2005年   2353篇
  2004年   2253篇
  2003年   2110篇
  2002年   1927篇
  2001年   1800篇
  2000年   1716篇
  1999年   1377篇
  1998年   1470篇
  1997年   1387篇
  1996年   1100篇
  1995年   1142篇
  1994年   962篇
  1993年   872篇
  1992年   855篇
  1991年   759篇
  1990年   856篇
  1989年   717篇
  1988年   650篇
  1987年   814篇
  1986年   663篇
  1985年   855篇
  1984年   922篇
  1983年   862篇
  1982年   831篇
  1981年   707篇
  1980年   663篇
  1979年   606篇
  1978年   603篇
  1977年   552篇
  1976年   539篇
  1975年   499篇
  1974年   506篇
  1973年   468篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
101.
Zusammenfassung Nach zweijährigen Parallelregistrierungen der Windgeschwindigkeit und Windrichtung in Wien-Hohe Warte am Rande der Stadt Wien und an einer Meßstelle in der Stadtmitte wird gezeigt, daß ein merklicher und jahreszeitlich veränderlicher Umgebungseinfluß gerade am Stadtrand auf die Windgeschwindigkeit einwirkt. Während der Vegetationsperiode ist die Bodenrauhigkeit erhöht, die Windgeschwindigkeit in den unteren Stufenwerten bis etwa 35 km/h wird verringert. Während der vegetationslosen Zeit ist die Bodenrauhigkeit viel geringer, die Häufigkeitsverteilung der Windgeschwindigkeit im Winter daher viel normaler. Es besteht ein scharfer Gegensatz zwischen den Sommer-und Wintermonaten ohne langsame Übergänge. Das Ergebnis dieses zunächst lokalen Vergleiches ist von allgemeiner Bedeutung für Windbeobachtungen in den gemäßigten Breiten mit Vegetationswechsel.
Summary Based on two year's parallel observations of velocity and direction of wind at two stations, viz. the secular station Wien-Hohe Warte at the periphery and a station in the town-centre, it is shown that there exists a considerable and seasonally variable effect of local influences on the wind velocity, especially at the periphery of the town. During the vegetation period the roughness of the ground is increased and up to about 35 km/h the wind velocity is reduced. Out of the vegetation period the roughness of the ground is much smaller, the frequency distribution of wind velocity during the winter, therefore, shows more the normal features. There is a marked difference between the summer and winter months, and there exists no graduate change. The result of this local comparison seems to be of general interest to the climatology of wind in temperate latitudes with their seasonal change of vegetation.

Résumé Pendant deux ans on a enregistré les vitesses et les directions des vents dans le cadre d'observations faites simultanément à la périphérie de la ville de Vienne (station météorologique «Hohe Warte») et à une station située au centre de cette ville. Les résultats démontrent que c'est précisément à la périphérie de la ville que l'aspect du sol exerce une influence très nette, la vitesse des vents, qui varie selon les saisons. Pendant la saison de végétation la «rugosité» du terrain étant plus grande, les vents moins forts (jusqu'à 35 km/h) sont affaiblis. En hiver, quand il n'y a pas de végétation, la rugosité du sol est moindre, et par conséquent les fréquences respectives des vents d'intensités diverses offrent un tableau mieux équilibré. Entre les mois d'hiver et les mois d'été, le contraste est très brusque; il n'y a pas de période de lente transition. Le résultat de ces essais, effectués seulement sur un plan local jusqu'à présent, est d'importance générale pour l'étude des vents dans les régions de climat tempéré, avec une végétation changeante.


Mit 1 Textabbildung

Herrn Prof. Dr.H. Ficker zum 75. Geburtstag gewidmet.  相似文献   
102.
Analysis of the NWA 2086 CV3 chondrite showed a matrix/chondrule ratio of 52%, similar to Bali, Mokoia, and Grosanaja. Nearly twice as many chondrule fragments as intact ones demonstrate that an early fragmentation phase occurred prior to final accretion. After this event, no substantial mechanical change or redeposition is evident. Rims with double‐layered structures were identified around some chondrules, which, in at least one case, is attributed to an accretionary origin. The rim's outer parts with a diffuse appearance were formed by in situ chemical alteration. During this later process, Mg content decreased, Fe content increased, and olivine composition was homogenized, producing a rim composition close to that of the matrix. This alteration occasionally happened along fractures and at confined locations, and was probably produced by fluid interactions. Iron oxides are the best candidate for a small grain‐sized alteration product; however, technical limitations in the available equipment did not allow exact phase identification. These results suggest that NWA 2086 came from a location (possible more deeply buried) in the CV parent body than Mokoia or Bali, and suffered less impact effects—although there is no evidence of sustained thermal alteration. This meteorite may represent a sample of the CV parent asteroid interior and provide a useful basis for comparison with other CV meteorites in the future.  相似文献   
103.
The study of trace metal speciation has benefited from a great deal of interest leading to the development and the diversification of sequential extraction schemes (SES), which triggered the need for harmonization by the standard, measurements and testing programme (SM & T). However, some uncertainties still persist in the application of the harmonized 3-step protocol, because of the difficulty in conceptualizing a technique that can be applied to environmental samples irrespective of their nature. The alternative method proposed in this study is based on the solubility of the sample components progressively dissolved during the course of an acidimetric titration by 1 mol L−1 HCl. The major HCl-reactive mineralogical components are identified using mass balance calculation of H+ consumed by their dissolution together with the amount of major elements released into solution. The speciation of minor and trace elements is investigated by comparing their titrations to those of the major elements. This approach is much simpler than SES because it uses simple non-selective H+ at room temperature instead of a complex experimental design of so-called specific reagents. The different mineral components of the solid are no longer operationally defined and the problem of selectivity is irrelevant to the titration approach. The method was applied to several sediment samples from the Scheldt estuary and the particulate phase was further examined by Scanning Electron Microprobe and X-ray Diffraction techniques. The nearly complete consumption of H+ in the suspension is balanced by the total dissolution of carbonates and Fe-oxyhydroxides. In contrast to the speciation inferred from the Tessier SES, the acidimetric titration has demonstrated that the carbonate phase does not significantly contain trace metals with the exceptions of 40% of the Mn and 30% of the Co. In contrast, the Fe-oxyhydroxides seem to play a major role and account for 70% of Pb and 20% of Cr, in addition to 60% of P and additional amounts of 20% Co and 40% Mn. 70% of the Cu also occur in the oxyhydroxide phase, more likely coprecipitated with gibbsite. 90% of the Cd and 85% of Zn can be attributed to the Acid Volatile Sulfide (AVS) phase as evidenced from S titration. The acidimetric titration method not only provides information on the speciation of trace metals but also allows the quantification of their reactivity and mobility, if one considers that the titration roughly mimics pH changes that may occur as a result of chemical disequilibrium in the environment. The results demonstrate the potential of the acidimetric titration as an alternative to SES protocols in geochemical and environmental regulation studies. This method is applicable to a wide variety of environmental materials with little or minor adjustments.  相似文献   
104.
The intellection of seismic wave propagation in coal measures demands direct observation of the wavefield progression. Two vertical seismic profiles with high spatial and temporal sampling, were recently recorded in the Sydney Basin coalfields as part of an experimental coal seismic program. Static corrections and interval velocities were obtained by an automated system to determine first kicks and pulse rise times. Upgoing and downgoing waves were separated in the f—k-plane using a novel technique of contour slice filtering. The isolated upgoing waves clearly display reflections from the major coal seams within the stratigraphic sequence. The downgoing wave spectra were subjected to attenuation analysis. The deduced specific quality factor Q for Permian coal measure rocks lies in the range 20–70. Similar estimates were obtained in the time domain from measurements of pulse broadening. Synthetic VSP seismograms, computed using an exact recursive formulation, are an indispensable aid to interpretation. They illustrate the filtering effects of coal seams and sequences, and the effects of the contribution of internal and free-surface multiple reflections in the recorded wavetrains.  相似文献   
105.
106.
The causes of the high Mn concentration in the solid phase and pore solution of bottom sediments in the Mozhaisk Reservoir are discussed. Regularities are identified in variations the concentrations of Mn forms in reservoir deposits from its upper part to the dam.  相似文献   
107.
108.
109.
110.
Bumba  V.  Garcia  A.  Klvaňa  M. 《Solar physics》2000,197(1):175-202
The first small active regions of the last two new cycles seem to be formed, in its very first, preparatory stage, close to the equator with uncertain magnetic orientation, and as secondary products at the periphery of equatorial `magnetic bubbles' of the new magnetic flux still belonging to the old cycle. At the real beginning of the new cycle, at the periphery of its higher-latitude `magnetic bubbles', the opposite applies to the secondary regions of the ending cycle. It seems that two modes of magnetic flux supply the visible layers of the photosphere during the cycle transition phase: the emergence of the magnetic flux from the depth of the convective zone, and the mutual interaction of the earlier emerging fluxes, or the action of the `local dynamo', giving rise to the new local magnetic field concentrations.  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号