全文获取类型
收费全文 | 1951篇 |
免费 | 68篇 |
国内免费 | 15篇 |
专业分类
测绘学 | 38篇 |
大气科学 | 148篇 |
地球物理 | 404篇 |
地质学 | 751篇 |
海洋学 | 134篇 |
天文学 | 346篇 |
综合类 | 7篇 |
自然地理 | 206篇 |
出版年
2023年 | 9篇 |
2022年 | 7篇 |
2021年 | 25篇 |
2020年 | 29篇 |
2019年 | 20篇 |
2018年 | 45篇 |
2017年 | 28篇 |
2016年 | 52篇 |
2015年 | 42篇 |
2014年 | 48篇 |
2013年 | 125篇 |
2012年 | 55篇 |
2011年 | 96篇 |
2010年 | 84篇 |
2009年 | 103篇 |
2008年 | 98篇 |
2007年 | 75篇 |
2006年 | 82篇 |
2005年 | 74篇 |
2004年 | 77篇 |
2003年 | 77篇 |
2002年 | 79篇 |
2001年 | 52篇 |
2000年 | 43篇 |
1999年 | 52篇 |
1998年 | 51篇 |
1997年 | 28篇 |
1996年 | 23篇 |
1995年 | 23篇 |
1994年 | 30篇 |
1993年 | 29篇 |
1992年 | 25篇 |
1991年 | 21篇 |
1990年 | 24篇 |
1989年 | 30篇 |
1988年 | 14篇 |
1987年 | 12篇 |
1986年 | 17篇 |
1985年 | 21篇 |
1984年 | 26篇 |
1983年 | 19篇 |
1982年 | 19篇 |
1981年 | 27篇 |
1980年 | 22篇 |
1979年 | 16篇 |
1977年 | 10篇 |
1976年 | 12篇 |
1975年 | 7篇 |
1974年 | 12篇 |
1970年 | 8篇 |
排序方式: 共有2034条查询结果,搜索用时 328 毫秒
981.
Darren S. Madgwick Ed Hawkins Ofer Lahav Steve Maddox Peder Norberg John A. Peacock Ivan K. Baldry Carlton M. Baugh Joss Bland-Hawthorn Terry Bridges Russell Cannon Shaun Cole Matthew Colless Chris Collins Warrick Couch Gavin Dalton Roberto De Propris Simon P. Driver George Efstathiou Richard S. Ellis Carlos S. Frenk Karl Glazebrook Carole Jackson Ian Lewis Stuart Lumsden Bruce A. Peterson Will Sutherland Keith Taylor 《Monthly notices of the Royal Astronomical Society》2003,344(3):847-856
982.
Ian Carstairs 《Astronomy& Geophysics》2002,43(2):2.27-2.28
A two-day discussion meeting on the latest developments in X-ray astronomy was held on 19 and 20 February 2002 at the Royal Society, organized by Roger Blandford, Andy Fabian and Ken Pounds. Ian Carstairs reports. 相似文献
983.
Manuela Magliocchetti Steve J. Maddox Carole A. Jackson Joss Bland-Hawthorn Terry Bridges Russell Cannon Shaun Cole Matthew Colless Chris Collins Warrick Couch Gavin Dalton Roberto de Propris Simon P. Driver George Efstathiou Richard S. Ellis Carlos S. Frenk Karl Glazebrook Ofer Lahav Ian Lewis Stuart Lumsden John A. Peacock Bruce A. Peterson Will Sutherland Keith Taylor 《Monthly notices of the Royal Astronomical Society》2002,333(1):100-120
984.
985.
Nelson D. Padilla Carlton M. Baugh Vincent R. Eke Peder Norberg Shaun Cole Carlos S. Frenk Darren J. Croton Ivan K. Baldry Joss Bland-Hawthorn Terry Bridges Russell Cannon Matthew Colless Chris Collins Warrick Couch Gavin Dalton Roberto De Propris Simon P. Driver George Efstathiou Richard S. Ellis Karl Glazebrook Carole Jackson Ofer Lahav Ian Lewis Stuart Lumsden Steve Maddox Darren Madgwick John A. Peacock Bruce A. Peterson Will Sutherland Keith Taylor 《Monthly notices of the Royal Astronomical Society》2004,352(1):211-225
986.
987.
Ian Halliday Alan T. Blackwell Arthur A. Griffin 《Meteoritics & planetary science》1991,26(3):243-249
Abstract— Recent estimates of the current rate of meteorite falls have been derived from camera network observations and from the statistics of the recovery of small fragments in Roosevelt County, New Mexico. The results are discordant. The integrated sky coverage for the camera data is an order of magnitude greater than the long exposure over small areas in New Mexico, yet the number of inferred events is comparable. We examine potential problems and find no effects other than random ones to bias the camera data. New data on the total number of suitable fireballs indicate that the flux from the camera network is already close to the upper limit imposed by the count of over 700 fireballs. By contrast, the calibration of the decay time for small fragments in New Mexico appears insecure and could account for a factor-of-three discrepancy. The large area of a typical strewn field relative to the small search areas is also a serious problem that remains uncalibrated. There are problems with the application of either the camera results or the New Mexico data to the statistics of recoveries in Antarctica since the Antarctic search areas are not free from the strewn-field problem. Since there is no evidence for a substantial change in the infall rate in intervals less than the ages of the collecting surfaces, we believe the camera network flux data remain the best estimate for the arrival rate of small meteorites on Earth. 相似文献
988.
During the autumn of 2000, large areas of England and Wales were affected by severe flooding, which caused widespread disruption and significant damage to property. This study attempts to determine the impact of these flood events on contaminated sediment dispersal and deposition in the River Swale catchment, Yorkshire, UK, where lead and zinc were extracted and processed in large quantities during the nineteenth century. Seventy samples of overbank and channel‐edge sediments were collected at 35 sites along the River Swale. Inductively coupled plasma‐mass spectrometry was used to measure contaminant metal concentrations in the 2000–63 µm (sand) and <63 µm (silt and clay) size fractions. In both the channel‐edge and overbank sediments collected from the upper and middle reaches of the River Swale, concentrations of lead, zinc and cadmium were found to exceed MAFF guidelines. Highest concentrations correspond to the input of contaminated material from intensively mined tributaries, and elevated levels can be observed 5–10 km downstream of these inputs. This indicates that the remobilization of contaminated material during major flood events is potentially a serious problem for activities such as agriculture that utilize the Swale floodplain. Copyright © 2003 John Wiley & Sons, Ltd. 相似文献
989.
Ian D. Howarth Keith C. Smith† 《Monthly notices of the Royal Astronomical Society》2001,327(2):353-368
We present N -body simulations of galaxy groups embedded in a common halo of matter. We study the influence of the different initial conditions upon the evolution of the group and show that denser configurations evolve faster, as expected. We then concentrate on the influence of the initial radial density profile of the common halo and of the galaxy distribution. We select two kinds of density distributions, a singular profile (modelled by a Hernquist distribution) and a profile with a flat core (modelled by a Plummer sphere). In all cases we witness the formation of a central massive object owing to mergings of individual galaxies and to accretion of stripped material, but both its formation history and its properties depend heavily on the initial distribution. In Hernquist models the formation is caused by a 'burst' of mergings in the inner parts, owing to the large initial concentration of galaxies in the centre. The merging rate is much slower in the initial phases of the evolution of a Plummer distribution, where the contribution of accretion to the formation of the central object is much more important. The central objects formed within Plummer distributions have projected density profiles which are not in agreement with the radial profiles of observed brightest cluster members, unless the percentage of mass in the common halo is small. In contrast, the central object formed in initially cusped models has projected radial profiles in very good agreement with those of brightest cluster members, sometimes also showing luminosity excess over the r 1/4 law in the outer parts, as is observed in cD galaxies. 相似文献
990.