全文获取类型
收费全文 | 41422篇 |
免费 | 590篇 |
国内免费 | 318篇 |
专业分类
测绘学 | 959篇 |
大气科学 | 2944篇 |
地球物理 | 8001篇 |
地质学 | 14216篇 |
海洋学 | 3848篇 |
天文学 | 9741篇 |
综合类 | 74篇 |
自然地理 | 2547篇 |
出版年
2021年 | 404篇 |
2020年 | 401篇 |
2019年 | 453篇 |
2018年 | 940篇 |
2017年 | 843篇 |
2016年 | 1090篇 |
2015年 | 608篇 |
2014年 | 1001篇 |
2013年 | 2073篇 |
2012年 | 1132篇 |
2011年 | 1619篇 |
2010年 | 1470篇 |
2009年 | 1983篇 |
2008年 | 1645篇 |
2007年 | 1730篇 |
2006年 | 1587篇 |
2005年 | 1311篇 |
2004年 | 1270篇 |
2003年 | 1241篇 |
2002年 | 1193篇 |
2001年 | 1056篇 |
2000年 | 980篇 |
1999年 | 810篇 |
1998年 | 813篇 |
1997年 | 829篇 |
1996年 | 668篇 |
1995年 | 656篇 |
1994年 | 616篇 |
1993年 | 570篇 |
1992年 | 526篇 |
1991年 | 495篇 |
1990年 | 506篇 |
1989年 | 496篇 |
1988年 | 474篇 |
1987年 | 553篇 |
1986年 | 489篇 |
1985年 | 604篇 |
1984年 | 650篇 |
1983年 | 592篇 |
1982年 | 527篇 |
1981年 | 577篇 |
1980年 | 469篇 |
1979年 | 458篇 |
1978年 | 433篇 |
1977年 | 433篇 |
1976年 | 383篇 |
1975年 | 378篇 |
1974年 | 376篇 |
1973年 | 384篇 |
1971年 | 224篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
301.
302.
The eclipsing binary AV Hya has been observed photoelectrically inU, B andV filters on 15 nights. The primary eclipse appeared to be total with a totality of 23 min duration. A modified period of 0d.6 834 062 has been obtained. Geometrical elements could only be determined for partial transit case. 相似文献
303.
In this paper we give a detailed general relativistic formulation of the study of structure and stability of charged fluid
disks around compact objects like black holes neglecting the self-gravitation of the disk itself. Having presented the general
equations for equilibrium as well as for perturbations we solve explicitly the cases of rigidly and differentially rotating
thin disks, with constant charge density and zero pressure, confined to the equatorial plane of the black hole. By using normal
mode analysis we have analysed the stability of such disks under purely radial perturbations and find that the disks are generally
stable.
On leave of absence from Government College, Jagadalpur 494005 相似文献
304.
The seasonal variation of the nocturnal average intensity, and the typical variation of the sodium airglow intensity during the night have been deduced, using a data set that has been accumulated over a period of 5 years. The maximum intensity, which occurs at the equinoxes, is about 2–3 times as large as the intensity during winter, when the intensity of the D2 line is about 30 R. The nocturnal variation is symmetrical about midnight, where the intensity is some 30% less than just after (before) dusk (dawn) values. 相似文献
305.
Following the recent mass spectrometric observations of the ambient stratospheric positive and negative ions we have carried out co-ordinated laboratory experiments using a selected ion flow tube apparatus and a flowing afterglow apparatus for the following purposes: (i) to consider whether CH3CN is a viable candidate molecule for the species X in the observed stratospheric ion series H+ (H2On (X)m and (ii) to determine the binary mutual neutralization rate coefficients αi for the reactions ofH+ (H2O4 and H+(H2O)(CH3CN)3 with several of the negative ion species observed in the stratosphere. We conclude from (i) that CH3CN is indeed a viable candidate for X and from (ii) that the αi for stratospheric ions are within the limited range (5–6) × 10?8 cm3 s?1. 相似文献
306.
Falconer David A. Jordan Stuart D. Brosius Jeffrey W. Davila Joseph M. Thomas Roger J. Andreatta Vicenzo Hara Hirohisa 《Solar physics》1998,180(1-2):179-191
We investigate the possibility that strong EUV lines observed with the Goddard Solar EUV Rocket Telescope and Spectrograph (SERTS) provide good proxies for estimating the total coronal flux over shorter wavelength ranges. We use coordinated SERTS and Yohkoh observations to obtain both polynomial and power-law fits relating the broad-band soft X-ray fluxes to the intensities of Fexvi 335 Ú and 361 Ú, Fexv 284 Ú and 417 Ú, and Mgix 368 Ú measured with SERTS. We found that the power-law fits best cover the full range of solar conditions from quiet Sun through active region, though not surprisingly the cooler Mgix 368 Ú line proves to be a poor proxy. The quadratic polynomial fits yield fair agreement over a large range for all but the Mgix line. However, the linear fits fail conspicuously when extrapolated into the quiet-Sun regime. The implications of this work for the Heii 304 Ú line formation problem are also briefly considered. 相似文献
307.
D. R. Bates 《Astrophysics and Space Science》1978,55(1):7-13
The problem of, attempting to make radio contact, with other technological civilizations is examined. It is argued that there are few (perhaps indeed no) omnidirectional radio beacons in the Galaxy primarily because any such beacon, to be effective, would have to be designed for a call-response time of at least some 104 years, which is much too long to be likely to be acceptable to governments. A consequence, is that any search program by us would have little chance of detecting incoming signals.Paper dedicated to Professor Hannes Alfvén on the occasion of his 70th birthday, 30th May, 1978. 相似文献
308.
We have conducted a targeted high-sensitivity search for narrow-band signals near γ18 cm using the 91-m radiotelescope of the National Radio Astronomy Observatory. The search included 201 nearby solar-type stars and achieved a frequency resolution of 5.5 Hz over a 1.4-MHz bandwidth. This high spectral Mark I VLBI recording terminal in conjunction with the CDC 7600 computational facility at the NASA-Ames Research Center. This is the first high-resolution search for narrow-band signals in this wavelength regime. To date it is the most sensitive search per unit observing time of any search strategy which does not postulate a unique magic frequency. Our data show no evidence for narrow-band signals due to extraterrestrial intelligence at a 12-σ upper limit on signal strength of 1.1 × 10?23 W m?2. 相似文献
309.
报告了中、美两国在喜马拉雅山区进行的第一次深反射地震试验的结果.试验剖面南起喜马拉雅山山脊南亚东县的帕里镇,向北穿过喜马拉雅山脊的荡拉,到达康马南的萨马达.剖面长约100km.共中心点(CMP)叠加剖面上显示出:1.在地壳中部有一强反射带,向北缓倾斜下去,延长达100km以上.它可能代表了一个活动的逆冲断裂或是一条巨大的拆离带,印度地壳整体或下地壳沿此拆离层俯冲到藏南之下.2.上部地壳的反射很丰富,显示了上地壳存在着大规模的叠瓦状结构.3.下地壳的反射同相轴呈现短而有规律的分布,显示了塑性流变特征.4.在测线南部莫霍反射明显,深度达72-75km.发现南部有双莫霍层的存在.5.试验中还取得莫霍层下面32,38,48s等双程走时的多条反射,向北倾斜,反射同相轴延续较长,信息丰富,反映了上地幔的成层结构和变形特征.这些结果对印度大陆地壳整体或其下地壳俯冲到藏南特提斯喜马拉雅地壳之下,并导致西藏南端地壳增厚的观点,给予了实质性的支持. 相似文献
310.
Energy transport in a hot flare plasma is examined with particular reference to the influence of fluid motion. On the basis of dimensional considerations the dynamical timescale of the flare plasma is shown to be comparable to the timescale for energy loss by conduction and radiation. It is argued that mass motion is likely to have a profound influence on the evolution of the flare.The detailed response of a flare filament to a localized injection of energy is then analyzed. Radiative, conductive and all dynamical terms are included in the energy equation. Apart from greatly enhancing the rate of propagation of the thermal disturbance through space, mass motion is found to be significant in transferring energy through the moving fluid.Finally the predicted thermal structure is discussed and it is concluded that the presence of mass motions in the flare may be inferred from the form of the soft X-ray differential emission measure. 相似文献