全文获取类型
收费全文 | 3580篇 |
免费 | 389篇 |
国内免费 | 283篇 |
专业分类
测绘学 | 1664篇 |
大气科学 | 160篇 |
地球物理 | 452篇 |
地质学 | 1068篇 |
海洋学 | 252篇 |
天文学 | 101篇 |
综合类 | 356篇 |
自然地理 | 199篇 |
出版年
2024年 | 1篇 |
2023年 | 15篇 |
2022年 | 124篇 |
2021年 | 166篇 |
2020年 | 162篇 |
2019年 | 169篇 |
2018年 | 89篇 |
2017年 | 227篇 |
2016年 | 235篇 |
2015年 | 235篇 |
2014年 | 238篇 |
2013年 | 245篇 |
2012年 | 235篇 |
2011年 | 224篇 |
2010年 | 155篇 |
2009年 | 181篇 |
2008年 | 181篇 |
2007年 | 202篇 |
2006年 | 174篇 |
2005年 | 146篇 |
2004年 | 115篇 |
2003年 | 101篇 |
2002年 | 89篇 |
2001年 | 66篇 |
2000年 | 60篇 |
1999年 | 62篇 |
1998年 | 43篇 |
1997年 | 55篇 |
1996年 | 55篇 |
1995年 | 38篇 |
1994年 | 33篇 |
1993年 | 15篇 |
1992年 | 23篇 |
1991年 | 15篇 |
1990年 | 24篇 |
1989年 | 9篇 |
1988年 | 15篇 |
1987年 | 13篇 |
1986年 | 7篇 |
1985年 | 3篇 |
1984年 | 1篇 |
1983年 | 2篇 |
1981年 | 2篇 |
1980年 | 1篇 |
1976年 | 1篇 |
排序方式: 共有4252条查询结果,搜索用时 265 毫秒
931.
932.
针对已有的特征点检测算法的不足,文章提出了一种基于自适应支撑区域(ROS)的算法,该算法针对目前特征点检测中的支撑区域选择,提出了一种自适应单调检测方法,改变了传统支撑区域选择过于单一的难点,自适应性强;并对于曲率的非极大值抑制易造成误检的问题,给出了三次扫描算法,即分析误检产生机理筛选候选特征点。通过支撑区域的自适应选择和三次扫描,实现了算法的自适应性和鲁棒性,检测精度高。试验结果表明,该算法无需先验参数,运行效率高,算法复杂度低。 相似文献
933.
地铁隧道三维激光扫描数据配准方法 总被引:1,自引:1,他引:0
针对传统的迭代最近点算法(ICP)用于多测站点云数据配准时计算效率低的问题,该文提出了一种基于特征点的ICP改进算法,该方法利用相邻两测站数据进行配准的实现。首先采用体素化格网方法对两点云数据集进行精简处理,并计算精简处理后每一点的法向量;然后利用kd-tree最近邻查询搜索特征点之间的对应关系;并通过估计出的最优变换矩阵更新至全局变换,以提高配准精度。实验结果表明,改进的ICP算法在地铁隧道点云数据配准中的效率高于其他的配准方法,为隧道变形监测工作的进行提供保证。 相似文献
934.
935.
针对三维激光扫描点云数据采集过密、冗余信息较多,现有压缩算法存在不足的问题,该文提出了基于点到平面距离的散乱点云压缩算法。将该算法与基于三角形法向量夹角和格网法两种现有算法的压缩结果进行比较,通过对比构建的空间三角网可以发现,该文算法对物体特征复杂的部位有较好的压缩效果,且在压缩率较高时,不会使较平缓的部位出现过度压缩而失真的情况。 相似文献
936.
937.
Nicolas Biver Dominique Bockelée-Morvan Jacques Crovisier Alain Lecacheux Gabriel Paubert Matthew Sumner Åke Hjalmarson Anders Winnberg Aage Sandqvist 《Icarus》2007,187(1):253-271
Comet 9P/Tempel 1 was the target of a multi-wavelength worldwide investigation in 2005. The NASA Deep Impact mission reached the comet on 4.24 July 2005, delivering a 370-kg impactor which hit the comet at 10.3 km s−1. Following this impact, a cloud of gas and dust was excavated from the comet nucleus. The comet was observed in 2005 prior to and after the impact, at 18-cm wavelength with the Nançay radio telescope, in the millimeter range with the IRAM and CSO radio telescopes, and at 557 GHz with the Odin satellite. OH observations at Nançay provided a 4-month monitoring of the outgassing of the comet from March to June, followed by the observation of H2O with Odin from June to August 2005. The peak of outgassing was found to be around between May and July. Observations conducted with the IRAM 30-m radio telescope in May and July 2005 resulted in detections of HCN, CH3OH and H2S with classical abundances relative to water (0.12, 2.7 and 0.5%, respectively). In addition, a variation of the HCN production rate with a period of 1.73±0.10 days was observed in May 2005, consistent with the 1.7-day rotation period of the nucleus. The phase of these variations, as well as those of CN seen in July by Jehin et al. [Jehin, E., Manfroid, J., Hutsemékers, D., Cochran, A.L., Arpigny, C., Jackson, W.M., Rauer, H., Schulz, R., Zucconi, J.-M., 2006. Astrophys. J. 641, L145-L148], is consistent with a rotation period of the nucleus of 1.715 days and a strong variation of the outgassing activity by a factor 3 from minimum to maximum. This also implies that the impact took place on the rising phase of the “natural” outgassing which reached its maximum ≈4 h after the impact. Post-impact observations at IRAM and CSO did not reveal a significant change of the outgassing rates and relative abundances, with the exception of CH3OH which may have been more abundant by up to one order of magnitude in the ejecta. Most other variations are linked to the intrinsic variability of the comet. The Odin satellite monitored nearly continuously the H2O line at 557 GHz during the 38 h following the impact on the 4th of July, in addition to weekly monitoring. Once the periodic variations related to the nucleus rotation are removed, a small increase of outgassing related to the impact is present, which corresponds to the release of ≈5000±2000 tons of water. Two other bursts of activity, also observed at other wavelengths, were seen on 23 June and 7 July; they correspond to even larger releases of gas. 相似文献
938.
Pramila Kumari Misra Sagarika Panigrahi P. Somasundaran 《International Journal of Mineral Processing》2006,80(2-4):229-237
The floatability of silica has been determined by adsorbing various concentrations of a series of polyoxyethylated nonyl and octyl alkyl phenols of varying oxyethylene units (10–40 units) to investigate the role of adsorbed layer. It is seen that the floatability of silica increases with increase in concentration till a maximum of 90% in premicellar region and then decrease to minimum of 40–45% in all cases in spite of the significant differences in adsorption densities. Zeta potential measurement reveals that a thin oxyethylene layer is formed at silica–water interface masking silica surface (Pramila K. Misra, P. Somasundaran, J. Surf. Deterg., Vol. 7, 2004, 373). This layer with oxyethylene units lying on silica surface and alkyl chain dangling to the bulk solution provides the same extent of hydrophobicity. The decrease in flotation recovery has been attributed to increase in the solvent hydrophobicity due to formation of premicellar aggregates and micelles. 相似文献
939.
940.
针对现有的相位梯度自聚焦(phase gradient autofocus,PGA)算法的加窗方法和特显点选取所存在的问题,提出一种改进的PGA算法。该算法提出一种新的确定相位误差点扩展函数支撑域的方法,此方法计算方位向上能量分布的平均值作为支撑域外的平均能量,以此来确定加窗的宽度。基于这种自适应加窗方法,还提出一种改进的特显点选取方法,该方法能够选择信杂比大的特显点,去掉信杂比小的特显点。试验结果表明,与传统的加窗方法和特显点选取方法相比,该方法能够得到更好的聚焦效果。 相似文献