全文获取类型
收费全文 | 132915篇 |
免费 | 2188篇 |
国内免费 | 992篇 |
专业分类
测绘学 | 3130篇 |
大气科学 | 9342篇 |
地球物理 | 25934篇 |
地质学 | 47230篇 |
海洋学 | 11777篇 |
天文学 | 30108篇 |
综合类 | 366篇 |
自然地理 | 8208篇 |
出版年
2021年 | 1263篇 |
2020年 | 1427篇 |
2019年 | 1571篇 |
2018年 | 3261篇 |
2017年 | 3029篇 |
2016年 | 3650篇 |
2015年 | 2033篇 |
2014年 | 3628篇 |
2013年 | 6795篇 |
2012年 | 3895篇 |
2011年 | 5201篇 |
2010年 | 4699篇 |
2009年 | 6046篇 |
2008年 | 5350篇 |
2007年 | 5449篇 |
2006年 | 5064篇 |
2005年 | 3919篇 |
2004年 | 3847篇 |
2003年 | 3644篇 |
2002年 | 3475篇 |
2001年 | 3104篇 |
2000年 | 3013篇 |
1999年 | 2586篇 |
1998年 | 2592篇 |
1997年 | 2452篇 |
1996年 | 2105篇 |
1995年 | 2063篇 |
1994年 | 1841篇 |
1993年 | 1729篇 |
1992年 | 1605篇 |
1991年 | 1633篇 |
1990年 | 1675篇 |
1989年 | 1493篇 |
1988年 | 1388篇 |
1987年 | 1630篇 |
1986年 | 1412篇 |
1985年 | 1794篇 |
1984年 | 2057篇 |
1983年 | 1969篇 |
1982年 | 1833篇 |
1981年 | 1716篇 |
1980年 | 1530篇 |
1979年 | 1484篇 |
1978年 | 1453篇 |
1977年 | 1307篇 |
1976年 | 1258篇 |
1975年 | 1211篇 |
1974年 | 1235篇 |
1973年 | 1259篇 |
1972年 | 786篇 |
排序方式: 共有10000条查询结果,搜索用时 457 毫秒
781.
DAVID A. ROTHERY 《Geology Today》1986,2(6):171-175
In January 1986 the spaceprobe Voyager-2 revealed details of the surfaces of the icy satellites of Uranus for the first time, including grabens, other faulted features, impact craters and possible ice flows. Despite their apparent similarity to some of the moons of Jupiter and Saturn, they highlight many new questions as to the evolution of, and interactions between, such bodies. 相似文献
782.
An analytical model for the constant-head pumping test is developed for a partially penetrating well that has a finite thickness skin, and intersects a single vertical fracture. In the model, the fracture is fully confined and flow occurs only in the fracture. The model is developed using Laplace transform and finite Fourier transform methods. The model is to be used for analysing well test data from vertically fractured media and for verifying numerical models. Dimensionless curves are used to study the effects of a finite thickness skin and a partially penetrating wellbore. In the presence of a finite thickness skin, or a partially penetrating wellbore, a typical flow response for the constant-head pumping test has three distinct periods of flow corresponding to small-, intermediate- and large-time. Small- and large-time approximations are presented for the model. For tests where the wellbore is fully penetrating, or the partial penetration ratio is known, these approximations can be used to analyse field data. 相似文献
783.
R. W. Komm 《Solar physics》1995,157(1-2):45-50
I analyze a quiet-Sun magnetogram with an orthogonal wavelet transform, which allows me to define an entropy measure. The entropy measure of the magnetogram as a function of spatial scale obeys a scaling law, which leads to a fractal dimension ofD
f
= 1.7. Furthermore, the entropy scaling law is directly related to the intermittency of magnetic features, which increases for decreasing spatial scales, as expected for a turbulent signal. In this context, the scaling law parameter can be interpreted as a fractional reduction in volume from one step of the turbulent cascade to the next.Operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation. 相似文献
784.
S. M. Matz J. E. Grove W. N. Johnson J. D. Kurfess G. H. Share G. J. Fishman C. A. Meegan 《Astrophysics and Space Science》1995,231(1-2):127-130
The BATSE and OSSE instrument teams have modified flight software to promptly (within 2 min of trigger) slew the OSSE detectors to burst locations determined on-board by BATSE. This enables OSSE to make sensitive searches for prompt and delayed post-burst line and continuum emission above 50 keV. In the best cases our sensitivity will be more than an order of magnitude better than any other search in this energy range. We expect to slew to 1–2 bursts per month, based on the OSSE FOV and BATSE event rate. Detections or limits from continued operation of this system may provide significant constraints on burst models. As an example of the observations made using this system, we present preliminary limits for post-burst emission from GRB 950223 on several time scales. 相似文献
785.
786.
Response of reef coral communities to sea-level rise: a Holocene model from Mauritius (Western Indian Ocean) 总被引:1,自引:0,他引:1
The fringing reef at Pointe-au-Sable (Mauritius, Indian Ocean) was used to examine the effects of Holocene sea-level rise on coral growth. This reef is about 1000 m wide and comprises a forereef slope (30 m maximum depth), a narrow reef crest and a very shallow backreef (1·5 m maximum depth). Four major coral communities were recognized, which developed within relatively narrow depth ranges: a Pachyseris/Oulophyllia community (deeper than 20 m), an Acropora‘tabulate’Faviid community (20–6 m); a robust branching Acropora community (less than 6 m) and a Pavona community (less than 10m). Three high-recovery cores show the Holocene reef sequence is a maximum of 19·3 m thick and comprises four coral biofacies which are similar to counterparts identified in modern communities: robust branching, tabular-branching, robust branching-domal and foliaceous coral facies. A minimum sea-level curve for the past 7500 years was constructed. Using distribution patterns of coral biofacies and radiocarbon dates from corals, reconstruction of reef growth history indicates that both offshore and onshore reef zones were developing coevally, aggrading at rates of 4·3 mm year?1 from 6900 years B.P. The reef caught up with sea-level only after sea-level stabilized. Changes in coral community and reef growth rates were driven principally by increasing water agitation due to the decrease in accommodation space. Based on the composition of the successive coral assemblages, the reef appears to have grown through successive equilibrium stages. 相似文献
787.
The subtle interactions between the magnetohydrodynamics (MHD) and transverse plasmons are investigated. It is shown that there is a resistive instability by the plasmon's soliton in a current sheet, which eventually turns into an eruptive instability at the magnetic field reconnection. In the case of ion-acoustic turbulence, the high temperature current sheet model must adopt the aromalous conductivity instead of the Coulomb conductivity. The numerical results are consistent with the observations obtained by Hanaoka (1994). Thus the flare caused by X-ray loop coalescence can be basically interpreted by this model of magnetic field reconnection driven by ponderomotive force. 相似文献
788.
P. Persi M. Ferrari-Toniolo A. R. Marenzi M. Busso L. Corcione M. Marengo M. Tapia 《Astrophysics and Space Science》1995,224(1-2):535-536
We present the results of direct mid-IR images of the luminous young stellar objects GL 2591, S140-IRS1, and W51-IRS2. The sources show an extended mid-IR emission at the limit of our spatial resolution indicating the presence of dense circumstellar dust disks. 相似文献
789.
Isabella A. Abbott 《中国海洋湖沼学报》1995,(4)
A new species of Liagora,L.perennis sp.nov.from Hawai’i,is described.Unlike dpecies of this genus in China,it is carpotetrasporangial,and at the place of expected carposporangia bears cruciately di-vided tetrasporangia,a detail which differentiates it from the usual species of Liagora without tetraspores that have been reported in China.Notes are provided on other Liagora species that have an impact on the taxonomy of species found in China. 相似文献
790.
P. MAISONGRANDE A. RUIMY G. DEDIEU B. SAUGIER 《Tellus. Series B, Chemical and physical meteorology》1995,47(1-2):178-190