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21.
GPS技术在金川露天矿边坡变形监测中的应用 总被引:6,自引:0,他引:6
本文结合金川露天矿边坡变形GPS监测研究,主要论述监测基点的选择,基点WGS-84坐标的确定,变形监测网的布设,GPS数据采集、处理和质量,坐标转换的实施等,给出反演推出的若干四等三角点及其它控制点的变形数据,这些数据和造成变形的物理成因符合得很好,最后概括出GPS技术应用于变形观测的若干优点。 相似文献
22.
Witold Maciejewski James Binney 《Monthly notices of the Royal Astronomical Society》2001,323(4):831-838
We consider long-slit emission-line spectra of galactic nuclei when the slit is wider than the instrumental point spread function, and the target has large velocity gradients. The finite width of the slit generates complex distributions of brightness at a given spatial point in the measured spectrum, which can be misinterpreted as coming from additional physically distinct nuclear components. We illustrate this phenomenon for the case of a thin disc in circular motion around a nuclear black hole (BH). We develop a new method for estimating the mass of the BH that exploits a feature in the spectrum at the outer edge of the BH's sphere of influence, and therefore gives higher sensitivity to BH detection than traditional methods. Moreover, with this method we can determine the BH mass and the inclination of the surrounding disc separately, whereas the traditional approach to BH estimation requires two long-slit spectra to be taken. We show that, with a given spectrograph, the detectability of a BH depends on the sense of rotation of the nuclear disc. We apply our method to estimate the BH mass in M84 from a publicly available spectrum, and recover a value four times lower than that published previously from the same data. 相似文献
23.
针对WGS-84CGCS2000坐标基准差异问题,分析了用于估计基准转换参数的Bursa模型及其求解方法,初步尝试求取WGS-84CGCS2000的坐标基准转换参数。算例采用了中国区域内含有CGCS2000坐标值,同时安装有GPS接收机的21个观测站,并针对点位的区域分布问题,提出利用重心化的Bursa模型求解转换参数的思路,且得到一组较好的转换结果。 相似文献
24.
一种快速获取GPS控制网精确WGS-84坐标方法 总被引:1,自引:0,他引:1
详细介绍了一种快速求取GPS控制网的精确WGS-84坐标的方法。首先选择三个天空通视条件较好、分布合理的控制网点,与附近的IGS跟踪站进行长基线相对定位或者直接进行静态精密单点定位,求得三点精确的WGS-84坐标,然后将这三个点作为已知点在WGS-84坐标系下进行三维约束平差,可求得控制网其它点精确的WGS-84坐标,这样求得网点的WGS-84坐标具有厘米级精度。 相似文献
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3C 84 is a well-known supermassive black hole that can be used to explore jet and accretion physics. In this work, we model the multiwavelength spectral energy distribution (SED) of the 3C 84, and find that the SED is difficult to fit with pure advection dominated accretion flow (ADAF) or pure jet model. Using a coupled ADAF-jet model to fit the SED of 3C 84, it is found that the radio emission and the millimeter emission can be naturally reproduced by the synchrotron radiation of nonthermal electrons in the jet, and that the X-ray emission may predominantly come from inverse Compton radiation from electrons in ADAF. According to the Rotation Measure (RM) obtained by the polarization observation, we consider the possible location of the polarizing source and found that the calculated RM in the jet is roughly consistent with the observational constraints. These results will help us better understand jets produced by black holes. 相似文献
28.
Position and velocity perturbations for the determination of geopotential from space geodetic measurements 总被引:10,自引:0,他引:10
Peiliang Xu 《Celestial Mechanics and Dynamical Astronomy》2008,100(3):231-249
Although space geodetic observing systems have been advanced recently to such a revolutionary level that low Earth Orbiting
(LEO) satellites can now be tracked almost continuously and at the unprecedented high accuracy, none of the three basic methods
for mapping the Earth’s gravity field, namely, Kaula linear perturbation, the numerical integration method and the orbit energy-based
method, could meet the demand of these challenging data. Some theoretical effort has been made in order to establish comparable
mathematical modellings for these measurements, notably by Mayer-Gürr et al. (J Geod 78:462–480, 2005). Although the numerical
integration method has been routinely used to produce models of the Earth’s gravity field, for example, from recent satellite
gravity missions CHAMP and GRACE, the modelling error of the method increases with the increase of the length of an arc. In
order to best exploit the almost continuity and unprecedented high accuracy provided by modern space observing technology
for the determination of the Earth’s gravity field, we propose using measured orbits as approximate values and derive the
corresponding coordinate and velocity perturbations. The perturbations derived are quasi-linear, linear and of second-order
approximation. Unlike conventional perturbation techniques which are only valid in the vicinity of reference mean values,
our coordinate and velocity perturbations are mathematically valid uniformly through a whole orbital arc of any length. In
particular, the derived coordinate and velocity perturbations are free of singularity due to the critical inclination and
resonance inherent in the solution of artificial satellite motion by using various types of orbital elements. We then transform
the coordinate and velocity perturbations into those of the six Keplerian orbital elements. For completeness, we also briefly
outline how to use the derived coordinate and velocity perturbations to establish observation equations of space geodetic
measurements for the determination of geopotential. 相似文献
29.
54与80坐标系转换数学模型研究 总被引:3,自引:0,他引:3
54北京坐标系与80西安坐标系转换计算,属54系与80系不同参考椭球下高斯—克吕格投影数据转换计算,因全国不同区域重力场的变化而无法用一个固定的参数或公式推算,能否另辟途径实现其精确算法。应用多元统计分析基础理论,研究二者互换随机数学模型,以福建省区域为例,成功实现大批数据坐标转换。 相似文献
30.