全文获取类型
收费全文 | 139381篇 |
免费 | 2075篇 |
国内免费 | 1889篇 |
专业分类
测绘学 | 4079篇 |
大气科学 | 9815篇 |
地球物理 | 26964篇 |
地质学 | 52050篇 |
海洋学 | 11687篇 |
天文学 | 28676篇 |
综合类 | 2458篇 |
自然地理 | 7616篇 |
出版年
2022年 | 770篇 |
2021年 | 1317篇 |
2020年 | 1402篇 |
2019年 | 1570篇 |
2018年 | 7542篇 |
2017年 | 6631篇 |
2016年 | 6042篇 |
2015年 | 2169篇 |
2014年 | 3684篇 |
2013年 | 6219篇 |
2012年 | 4665篇 |
2011年 | 7319篇 |
2010年 | 6281篇 |
2009年 | 7759篇 |
2008年 | 6721篇 |
2007年 | 7183篇 |
2006年 | 4800篇 |
2005年 | 3670篇 |
2004年 | 3845篇 |
2003年 | 3660篇 |
2002年 | 3430篇 |
2001年 | 2831篇 |
2000年 | 2737篇 |
1999年 | 2187篇 |
1998年 | 2276篇 |
1997年 | 2061篇 |
1996年 | 1823篇 |
1995年 | 1785篇 |
1994年 | 1533篇 |
1993年 | 1423篇 |
1992年 | 1369篇 |
1991年 | 1395篇 |
1990年 | 1388篇 |
1989年 | 1173篇 |
1988年 | 1124篇 |
1987年 | 1273篇 |
1986年 | 1152篇 |
1985年 | 1411篇 |
1984年 | 1584篇 |
1983年 | 1470篇 |
1982年 | 1377篇 |
1981年 | 1288篇 |
1980年 | 1181篇 |
1979年 | 1133篇 |
1978年 | 1079篇 |
1977年 | 915篇 |
1976年 | 898篇 |
1975年 | 882篇 |
1974年 | 844篇 |
1973年 | 913篇 |
排序方式: 共有10000条查询结果,搜索用时 0 毫秒
161.
This paper compares lead-acid batteries, sodium-sulfur batteries, solid polymer fuel cells and closed-cycle diesel engines for autonomous underwater vehicle (AUV) applications. The service is described in terms of a parametric mission and life cycle. A generic AUV is used as a basis for comparison. Power systems are evaluated by two criteria: (1) submerged endurance capability and (2) life cycle cost. This study determines categories of service for which each power system is preferred. The solid polymer fuel cell can provide greater submerged endurance than other power systems examined. For extremely long duration AUV missions, the fuel cell is the required system, indicating a possible market niche for today's fuel cell technology. Considering cost projections for each power system, the results also show that the SPFC can become cost-competitive with conventional technologies, particularly for services characterized by high levels of utilization 相似文献
162.
163.
Swath bathymetric, gravity, and magnetic studies were carried out over a 55 km long segment of the Central Indian Ridge.
The ridge is characterized by 12 to 15 km wide rift valley bounded by steep walls and prominent volcanic constructional ridges
on either side of the central rift valley. A transform fault at 7°45′S displaces the ridge axis. A mantle Bouguer anomaly
low of −14 mGals and shallowing of rift valley over the middle of the ridge segment indicate along axis crustal thickness
variations. A poorly developed neovolcanic zone on the inner rift valley floor indicate dominance of tectonic extension. The
off-axis volcanic ridgs suggest enhanced magmatic activity during the recent past.
Received: 24 May 1996 / Rivision received: 13 January 1997 相似文献
164.
We present special generating plane orbits, the vertical-critical orbits, of the coplanar general three-body problem. These
are determined numerically for various values of m3, for the entire range of the mass ratio of the two primaries. The vertical-critical orbits are necessary in order to specify
the vertically stable segments of the families of plane periodic orbits, and they are also the starting points of the families
of the simplest possible three-dimensional periodic orbits, namely the simple and double periodic. The initial conditions
of the vertical-critical periodic orbits of the basic families l, m, i, h, b and c and their stability parameters are determined.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
165.
An efficient and robust method has been developed to locate multiple impulsive sources in an ocean environment. Global position system (GPS) receivers were installed on sonobuoys to obtain their locations within a few meters of accuracy. A sonobuoy field was deployed in a ring-type pattern. Charges were then set off at arbitrary locations within the ring, High-resolution plots were used to obtain direct path and/or first bottom bounce arrivals on each buoy. A model grid of arrival times was constructed, corresponding to the dimensions of the buoy field. A ray model previously developed here at the Applied Research Laboratories at the University of Texas at Austin (ARL:UT) was used to obtain model travel times. The minimum value of the least-square-type error between the real arrival times and the modeled travel times resulted in an unambiguous location of the source, within the limits of the grid spacing chosen. This value was calculated by picking one receiver as the reference and then summing the timing errors of the remaining receivers relative to the reference. Successive iterations with finer grid spacings result in source localization within the accuracy of the buoy locations. The localization routine was extended by allowing permutations of the pulse arrivals on each buoy to account for multiple sources closely separated in time and/or space. An automated correlation technique is presented as an alternative to the leading edge-detection method used here for obtaining relative arrival times. Two proof-of-concept experiments were performed and some results of data obtained at Lake Travis and the Gulf of Mexico are presented 相似文献
166.
167.
We study the temporal intensity variations of Mgib bright features and investigate the corresponding Hα velocity pattern.
The network bright features are well visible in the continuum, in images averaged over the duration of the observations (130 min).
We detected `flashing' bright features, which appear and disappear within two to five minutes, while the rest of the bright
features undergo small variations of either their shape and/or their intensity. A power spectrum analysis reveals a 10-min
oscillation for approximately half of the stable bright features. The 5-min oscillations are detected mainly at the network
boundaries, where stable bright features are located, while 3-min oscillations coincide with few bright features, but are
also quite intense inside the network cells. The majority of bright features are associated with Hα downflows. The downflow
is very intense at the location of `flashing' bright features. 相似文献
168.
169.
170.
Nonlinear Alfvén wave in a hot rotating and strongly magnetized electron-positron plasma is considered. Using relativistic two fluid equations, the dispersion relation for Alfvén wave in the rotating plasma is obtained. Large amplitude Alfvén solitons are found to exist in the rotating pulsar plasma. Rotational effects on solitons are discussed. 相似文献