全文获取类型
收费全文 | 1031篇 |
免费 | 88篇 |
国内免费 | 252篇 |
专业分类
测绘学 | 288篇 |
大气科学 | 16篇 |
地球物理 | 148篇 |
地质学 | 486篇 |
海洋学 | 129篇 |
天文学 | 144篇 |
综合类 | 125篇 |
自然地理 | 35篇 |
出版年
2024年 | 1篇 |
2023年 | 6篇 |
2022年 | 21篇 |
2021年 | 16篇 |
2020年 | 25篇 |
2019年 | 22篇 |
2018年 | 19篇 |
2017年 | 40篇 |
2016年 | 41篇 |
2015年 | 45篇 |
2014年 | 38篇 |
2013年 | 44篇 |
2012年 | 54篇 |
2011年 | 69篇 |
2010年 | 48篇 |
2009年 | 64篇 |
2008年 | 63篇 |
2007年 | 82篇 |
2006年 | 66篇 |
2005年 | 63篇 |
2004年 | 49篇 |
2003年 | 45篇 |
2002年 | 39篇 |
2001年 | 42篇 |
2000年 | 36篇 |
1999年 | 38篇 |
1998年 | 40篇 |
1997年 | 15篇 |
1996年 | 28篇 |
1995年 | 25篇 |
1994年 | 34篇 |
1993年 | 32篇 |
1992年 | 19篇 |
1991年 | 42篇 |
1990年 | 35篇 |
1989年 | 5篇 |
1988年 | 8篇 |
1987年 | 6篇 |
1986年 | 2篇 |
1985年 | 1篇 |
1984年 | 1篇 |
1981年 | 1篇 |
1977年 | 1篇 |
排序方式: 共有1371条查询结果,搜索用时 503 毫秒
21.
The impact of accelerometry on CHAMP orbit determination 总被引:6,自引:0,他引:6
The contribution of the STAR accelerometer to the CHAMP orbit precision is evaluated and quantified by means of the following
results: orbital fit to the satellite laser ranging (SLR) observations, GPS reduced-dynamic vs SLR dynamic orbit comparisons,
and comparison of the measured to the modeled non-gravitational accelerations (atmospheric drag in particular). In each of
the four test periods in 2001, five CHAMP arcs of 2 days' length were analyzed. The mean RMS-of-fit of the SLR observations
of the orbits computed with STAR data or the non-gravitational force model were 11 and 24 cm, respectively. If the accelerometer
calibration parameters are not known at least at the few percent level, the SLR orbit fit deteriorates. This was tested by
applying a 10% error to the along-track scale factor of the accelerometer, which increased the SLR RMS-of-fit on average to
17 cm. Reference orbits were computed employing the reduced-dynamic technique with GPS tracking data. This technique yields
the most accurate orbit positions thanks to the estimation of a large number of empirical accelerations, which compensate
for dynamic modeling errors. Comparison of the SLR orbits, computed with STAR data or the non-gravitational force model, to
the GPS-based orbits showed that the SLR orbits employing accelerometer observations are twice as accurate. Finally, comparison
of measured to modeled accelerations showed that the level of geomagnetic activity is highly correlated with the atmospheric
drag model error, and that the largest errors occur around the geomagnetic poles.
Received: 7 May 2002 / Accepted: 18 November 2002
Correspondence to: S. Bruinsma
Acknowledgments. The TIGCM results were obtained from the CEDAR database. This study was supported by the Centre National d'Etudes Spatiales
(CNES). The referees are thanked for their helpful remarks and suggestions. 相似文献
22.
Geoid determination using adapted reference field, seismic Moho depths and variable density contrast 总被引:4,自引:0,他引:4
The traditional remove-restore technique for geoid computation suffers from two main drawbacks. The first is the assumption
of an isostatic hypothesis to compute the compensation masses. The second is the double consideration of the effect of the
topographic–isostatic masses within the data window through removing the reference field and the terrain reduction process.
To overcome the first disadvantage, the seismic Moho depths, representing, more or less, the actual compensating masses, have
been used with variable density anomalies computed by employing the topographic–isostatic mass balance principle. In order
to avoid the double consideration of the effect of the topographic–isostatic masses within the data window, the effect of
these masses for the used fixed data window, in terms of potential coefficients, has been subtracted from the reference field,
yielding an adapted reference field. This adapted reference field has been used for the remove–restore technique. The necessary
harmonic analysis of the topographic–isostatic potential using seismic Moho depths with variable density anomalies is given.
A wide comparison among geoids computed by the adapted reference field with both the Airy–Heiskanen isostatic model and seismic
Moho depths with variable density anomaly and a geoid computed by the traditional remove–restore technique is made. The results
show that using seismic Moho depths with variable density anomaly along with the adapted reference field gives the best relative
geoid accuracy compared to the GPS/levelling geoid.
Received: 3 October 2001 / Accepted: 20 September 2002
Correspondence to: H.A. Abd-Elmotaal 相似文献
23.
火焰原子吸收法间接测定磷矿中氯 总被引:2,自引:0,他引:2
火焰原子吸收法间接测定磷矿中氯达刘生1云南个旧市化肥厂中心化验室个旧661411目前磷矿中Cl-含量的测定多采用浊度法、氯离子选择电极法及离子色谱法。本文采用火焰原子吸收法来间接测定磷矿中Cl-,即在试样溶液中加入定量的Ag+,试样中Cl-与Ag+生... 相似文献
24.
25.
测氡法快速确定油气田边界及深度 总被引:5,自引:0,他引:5
叶树林 《华东地质学院学报》1996,19(2):150-156
本介绍了运用测氡法快速确定大庆××油气田边界,估算其埋藏深度试验,结果表明,该方法具有可行性和实用性。由于所做工作有限,尚属经验性探讨,还必须从理论和实践上进一步地工作,进而充实、完善它。 相似文献
26.
文章主要介绍应用 X射线荧光现场取样技术在新疆喀拉通克铜镍矿井下现场测定铜镍品位 ,快速评价矿石质量和降低工人劳动强度的方法和效率 相似文献
27.
热液矿床石英铅同位素组成及其地质意义 总被引:1,自引:0,他引:1
作者以若尔盖铀矿床为例,研究了含矿热液形成的石英脉石英的铅同位素组成,并将其作为联系母源铅同位素组成的桥梁,判别铀的来源。结果表明,矿床中石英铅同位素组成与含矿黄铁矿和中酸性构造-岩浆成因的花岗岩铅同位素组成具线性演化关系。由此提出含矿热液中的铀来自中酸性构造-岩浆岩而不是地层岩石的新见解,同时提出利用热液石英铅同位素组成判别非放射性矿床成矿元素来源的可能性。 相似文献
28.
本文详细论述了微波焙烧炉代替马弗炉应用于样品焙烧、熔融、活性炭灰化工作中的实际效果。结果表明:其应用不但可行,而且与马弗炉相比,微波焙烧炉具有更加优越的经济性与环保效果。 相似文献
29.
药用滑石粉酸中可溶物测定方法考察 总被引:1,自引:0,他引:1
考察药用滑石粉酸中可溶物测定方法的重复性、耐用性 ,分析主要影响因素。比较酸溶物提取液滤过介质对测定结果差异的影响 ;采用重量法随机测定酸溶物含量和室间差异。两种滤过介质处理对测定结果没有显著差异 ;室间测定结果没有显著差异 ;30批样品平行测定结果的 RSD值范围为 0 %~ 18.2 %。酸中可溶物测定法存在重复性和耐用性不佳的问题 ,应相应调整酸中可溶物含量限度 相似文献
30.