全文获取类型
收费全文 | 100351篇 |
免费 | 1548篇 |
国内免费 | 953篇 |
专业分类
测绘学 | 2697篇 |
大气科学 | 7109篇 |
地球物理 | 20477篇 |
地质学 | 34955篇 |
海洋学 | 8640篇 |
天文学 | 22914篇 |
综合类 | 297篇 |
自然地理 | 5763篇 |
出版年
2021年 | 926篇 |
2020年 | 1037篇 |
2019年 | 1128篇 |
2018年 | 2542篇 |
2017年 | 2373篇 |
2016年 | 3022篇 |
2015年 | 1754篇 |
2014年 | 2891篇 |
2013年 | 5203篇 |
2012年 | 3065篇 |
2011年 | 4159篇 |
2010年 | 3577篇 |
2009年 | 4814篇 |
2008年 | 4351篇 |
2007年 | 4222篇 |
2006年 | 3964篇 |
2005年 | 3144篇 |
2004年 | 3082篇 |
2003年 | 2866篇 |
2002年 | 2754篇 |
2001年 | 2523篇 |
2000年 | 2399篇 |
1999年 | 1972篇 |
1998年 | 2070篇 |
1997年 | 2005篇 |
1996年 | 1610篇 |
1995年 | 1611篇 |
1994年 | 1396篇 |
1993年 | 1288篇 |
1992年 | 1188篇 |
1991年 | 1141篇 |
1990年 | 1205篇 |
1989年 | 1099篇 |
1988年 | 983篇 |
1987年 | 1182篇 |
1986年 | 1017篇 |
1985年 | 1262篇 |
1984年 | 1417篇 |
1983年 | 1312篇 |
1982年 | 1269篇 |
1981年 | 1123篇 |
1980年 | 1020篇 |
1979年 | 963篇 |
1978年 | 972篇 |
1977年 | 856篇 |
1976年 | 821篇 |
1975年 | 798篇 |
1974年 | 771篇 |
1973年 | 782篇 |
1972年 | 537篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
981.
M. Stepanova T. Vucina-Parga E. Antonova I. Ovchinnikov Y. Yermolaev 《Journal of Atmospheric and Solar》2005,67(17-18):1815
Fluctuations of the plasma bulk velocity across the plasma sheet are studied using single-point measurements from the Corall instrument on board the Interball/Tail satellite. Several hour-long intervals of continuous data corresponding to quiet geomagnetic conditions and different phases of isolated substorms are analyzed. The plasma sheet flow appears to be strongly turbulent, i.e. dominated by fluctuations that are unpredictable. Corresponding eddy diffusion coefficients were obtained as a function of the autocorrelation time and rms velocity of the fluctuations. It was found that the amplitude of the turbulence and the values of eddy-diffusion coefficients increase significantly during substorm growth and expansion phases and they decrease to their initial level during the recovery phase. We also studied a relationship between the eddy-diffusion coefficients and the absolute value of the geomagnetic field, also measured by the Interball/Tail satellite. It was found that this relationship varies depending on the phase of substorm, indicating possible change in the turbulence regimen with substorm phase. 相似文献
982.
983.
984.
985.
Edith L Gego P. Steven Porter John S. Irwin Christian Hogrefe S. Trivikrama Rao 《Pure and Applied Geophysics》2005,162(10):1919-1939
Airborne fine particulate matter across the United States is monitored by different networks, the three prevalent ones presently being the Clean Air Status and Trend Network (CASTNet), the Interagency Monitoring of PROtected Visual Environment Network (IMPROVE) and the Speciation and Trend Network (STN). If combined, these three networks provide speciated fine particulate data at several hundred locations throughout the United States. Yet, differences in sampling protocols and samples handling may not allow their joint use. With these concerns in mind, the objective of this study is to assess the spatial and temporal comparability of the sulfate, nitrate and ammonium concentrations reported by each of these networks. One of the major differences between networks is the sampling frequency they adopted. While CASTNet measures pollution levels on seven-day integrated samples, STN and IMPROVE data pertain to 24-hour samples collected every three days. STN and IMPROVE data therefore exhibit considerably more short-term variability than their CASTNet counterpart. We show that, despite their apparent incongruity, averaging the data with a window size of four to six weeks is sufficient to remove the effects of differences in sampling frequency and duration and allow meaningful comparison of the signals reported by the three networks of concern. After averaging, all the sulfate and, to a lesser degree, ammonium concentrations reported are fairly similar. Nitrate concentrations, on the other hand, are still divergent. We speculate that this divergence originates from the different types of filters used to collect particulate nitrate. Finally, using a rotated principal component technique (RPCA), we determined the number and the geographical organization of the significant temporal modes of variation (clusters) detected by each network for the three pollutants of interest. For sulfate and ammonium, the clusters’ geographical boundaries established for each network and the modes of variations within each cluster seem to correspond. RPCA erformed on nitrate concentrations revealed that, for the CASTNet and IMPROVE networks, the modes of variation do not correspond to unified geographical regions but are found more sporadically. For STN, the clustered areas are unified and easily delineable. We conclude that the possibility of jointly using the data collected by CASTNet, IMPROVE and STN has to be weighed pollutant by pollutant. While sulfate and ammonium data show some potential for joint use, at this point, combining the nitrate data from these monitoring networks may not be a judicious choice. 相似文献
986.
S. Y. Fu Q. G. Zong Z. Y. Pu C. J. Xiao A. Korth P. Daly H. Reme 《Surveys in Geophysics》2005,26(1-3):241-254
In this paper we report energetic ion behavior and its composition variations observed by the Cluster/RAPID instrument when the spacecraft was travelling in the high latitude magnetospheric boundary region on the day of the 31 March, 2001, strongest magnetic storm in the past 50 years. The Dst index reached −360 nT at about 09:00 UT. During its early recovery phase, large amounts of oxygen and helium ions were observed; the ratio of oxygen to hydrogen in the RAPID energy range reached as high as 250%, which suggests that the observed energetic particles might be of magnetospheric origin. The observations further show that enhanced energetic electron fluxes are confined in a very narrow region, while protons have occupied a larger region, and heavy ions have been observed in an even larger region. The flux of energetic electrons show a slight enhancement in a region where the magnetic field magnitude is around zero. These observed energetic ions could be quasi-trapped by the current sheet in the stagnation region of the cusp. 相似文献
987.
988.
J. Plomerova L. Vecsey V. Babuska M. Granet U. Achauer 《Studia Geophysica et Geodaetica》2005,49(4):541-560
We present results of an array study of seismic anisotropy beneath the Bohemian Massif (BM) showing distinct lateral and directional
variations of the fast shear-wave polarization and split-delay time consistent with variations in the P-residual spheres,
in which directional means of relative residuals are subtracted. Our analysis of the S- and P-wave anisotropy suggests that
the mantle lithosphere of the BM consists of at least three large domains with different orientation of the large-scale fabric
separated by sutures cutting most likely the whole lithosphere. Boundaries of the units are characterised by a null or small
shear-wave splitting, as well as by smaller values in the P-residual spheres. We present self-consistent 3D anisotropic models
of the lithosphere domains of the BM resulting from joint inversion of anisotropic parameters searching for a 3D orientation
of mantle fabric. While in the Saxothuringian and Sudetes parts of the BM the (a, c) foliations dip prevailingly to the N-NW,
they dip to the S and SW in the southern and eastern parts of the Moldanubian. 相似文献
989.
Comparative characteristic of several microelements (Ni, Cu, Sr, Al, Zn, Co, Mn, Pb, Cd, Hg, As) found in fish (case study of breams in the Volga basin reservoirs) is presented. Regularities of accumulation of these elements in fish depending on their concentration in the water are analyzed. Main disturbances in fish caused by the accumulation of microelements in their organs and tissues are considered. 相似文献
990.