共查询到20条相似文献，搜索用时 234 毫秒
1.
Poisson重力边值问题 总被引：1，自引：0，他引：1
提出了Ｐｏｉｓｓｉｏｎ重力边值问题,即关于扰动位的Ｐｏｉｓｓｏｎ方程的Ｓｔｏｋｅｓ问题和Ｎｅｕｍａｎｎ问题。作为导引,先研究Ｐｏｉｓｓｏｎ方程的Ｄｉｒｉｃｈｌｅｔ问题,再分别引入一种辅助函数,将Ｓｔｏｋｅｓ问题和Ｎｅｕｍａｎｎ问题改化为Ｄｉｒｉｃｈｌｅｔ问题,从而立即得到它们的积分解,最终解式表现为两部分叠加,一部分仪与边界观测相关,另一部分对地形测量的响应,为研究地形测量对外部重力场和大地水准面 相似文献
2.
地球外部扰动引力场确定的数据空间分布结构 总被引：1，自引：0，他引：1
在对各类平均重力异常的谱特征分析的基础上，通过对积分区外高频谱误差的估计，给出了在一定精度指标下各类平均重力异常数据积分区的分布；提出了一种反映局部重力场特征的重力异常阶方差模型。讨论了平均重力异常的重点力布设。本文研究的主题虽然是空中扰动引力确定的数据结构问题，但对于地面上的高程异常和垂线偏差确定具有相类似的参考作用。 相似文献
3.
用重力异常逐级余差计算重力大地水准面 总被引：1，自引：0，他引：1
本文将计算重力大地水准面的频域方法推广至空域，提出了一种新的用重力数据和重力模型位系数联合确定大地水准面的方法。利用重力异常的逐级余差实施积分，使得通常的Ｓｔｏｋｅｓ积分方法具有明确的频域分析含义，可按精度要求确定出使用重力异常余差的块形大小及积分半径ψｏ。 相似文献
4.
针对传统的均衡重力异常方式基于平面近似,积分范围较小、计算公式的适用性受限、表征的信息量有限的问题,该文在球坐标下分析艾黎-海斯卡宁(Airy-Hesikanen)均衡模型。以计算点向径为半径,将地形分为布格球壳和粗糙地形两部分,计算其地形影响和均衡改正。在实验区,选用补偿深度21km、密度差0.678g/cm3的模型参数,采用该文公式和传统公式计算均衡重力异常,并比较分析其计算值。结果表明,以球近似Airy-Hesikanen均衡模型计算均衡重力异常值,在小积分范围以及平坦地区,与传统公式计算值的精度相当;但随着积分半径增加,球近似Airy-Hesikanen均衡模型计算值精度不断提高、变化更平缓,说明球近似AiryHesikanen均衡模型代替平面近似Airy-Hesikanen均衡模型应用于重力问题研究更为符合地球实际情况。 相似文献
5.
空中测量地面平均重力异常的频域分析 总被引：6，自引：4，他引：6
本文首先给出了地面点重力异常代表误差的频域算式，进而将频域概念推广到空中重力异常的代表误差，推导出用空中一点重力异常代表地面一定块形平均重力异常的代表误差频域算式，据此可以讨论在空中测定地面平均重力异常的最佳高度。 相似文献
6.
针对Stokes-Pizzetti积分用于外部扰动重力场计算中从空中趋近地面时存在着不连续和积分奇异的问题,对该式进行了改进。改进式引入地面计算点处的重力异常,得到一个从地面到空中统一适用的公式,并且中和了在地面计算点处的奇异性。类似地,改进了的Stokes公式在用于大地水准面计算时积分的奇异性同样起到了改善作用。 相似文献
7.
基于物理大地测量边值问题的解,利用一阶边界算子定义,推导重力异常Δg、单层密度μ、大地水准面高N,垂线偏差ε、扰动重力δg等扰动场元的解。利用球谐函数的正交特性,通过对核函数的算子运算,可以得到上述扰动场元的有关逆变换公式。相对经典物理大地测量公式应用的边界面条件,笔者将含有因子r的对应扰动场元反演关系的公式称为广义积分公式。针对常用的重力异常Δg、大地水准面高N,垂线偏差ε、扰动重力δg计算,重点分析它们之间的变换关系,给出利用某个选定扰动场元计算其他扰动场元的广义积分公式。同时,通过对积分边界面的讨论,分析经典公式与广义积分公式的差异和联系。最后,给出所有外部扰动场元与核函数映射的关系表。 相似文献
8.
利用空中平均重力异常确定区域大地水准面 总被引：3，自引：0，他引：3
提出了直接利用空中平均重力异常计算区域大地水准面的方法。模拟计算的结果表明, 该方法与传统的利用地面平均空间重力异常确定的大地水准面精度相当, 但其显著优点是勿需空中重力异常的向下解析延拓, 从而可以避免延拓误差对大地水准面精化的影响。 相似文献
9.
针对局部重力异常向上延拓计算复杂、耗时长的问题,该文基于泊松积分离散化的基本原理,提出一种快速的局部格网重力异常向上延拓的实用算法;并结合中国东北和青藏高原地区大地水准面的重力异常格网数据,采用该延拓方法分别计算了空中10、50、100km处的重力异常,将其与等高度的EIGEN-6C4模型结果对比分析。实验结果表明:在顾及边界效应影响的情况下,相对于EIGEN-6C4模型,中国东北和青藏高原地区重力异常向上延拓的最大均方根误差分别优于1.5和3.5mGal;在保证精度可用的前提下,计算效率可以有大幅度提高,证明了该方法解算局部重力异常向上延拓的适用性。 相似文献
10.
分别采用基于梯度、基于泊松积分和基于快速傅里叶变换（FFT）的地面重力向上延拓方案,并提出交叉检验方法估计地面重力数据误差及其空中误差传播,对毛乌素测区GT-2A航空重力测量系统采集的空中测线数据进行外符合精度评价。对比结果表明：地面重力格网插值误差和代表性误差对空中点的影响达到0.66~0.92 mGal（1 Gal=1×10-2 m/s2）,航空重力数据误差估计必须扣除这一影响;基于泊松积分和基于FFT的地面重力向上延拓方法能够客观评价航空重力观测值的外符合精度,二者表现相当;扣除地面重力误差影响后,在包含残余边界效应的情况下,毛乌素测区GT-2A航空重力空中测线重力扰动的外符合精度优于1.42 mGal。 相似文献
11.
On the ellipsoidal correction to the spherical Stokes solution of the gravimetric geoid 总被引：2，自引：0，他引：2
The solutions of four ellipsoidal approximations for the gravimetric geoid are reviewed: those of Molodenskii et al., Moritz, Martinec and Grafarend, and Fei and Sideris. The numerical results from synthetic tests indicate that Martinec and Grafarends solution is the most accurate, while the other three solutions contain an approximation error which is characterized by the first-degree surface spherical harmonic. Furthermore, the first 20 degrees of the geopotential harmonic series contribute approximately 90% of the ellipsoidal correction. The determination of a geoid model from the generalized Stokes scheme can accurately account for the ellipsoidal effect to overcome the first-degree surface spherical harmonic error regardless of the solution used. 相似文献
12.
Far-zone effects for different topographic-compensation models based on a spherical harmonic expansion of the topography 总被引：1，自引：1，他引：0
The determination of the gravimetric geoid is based on the magnitude of gravity observed at the surface of the Earth or at
airborne altitude. To apply the Stokes’s or Hotine’s formulae at the geoid, the potential outside the geoid must be harmonic
and the observed gravity must be reduced to the geoid. For this reason, the topographic (and atmospheric) masses outside the
geoid must be “condensed” or “shifted” inside the geoid so that the disturbing gravity potential T fulfills Laplace’s equation everywhere outside the geoid. The gravitational effects of the topographic-compensation masses
can also be used to subtract these high-frequent gravity signals from the airborne observations and to simplify the downward
continuation procedures. The effects of the topographic-compensation masses can be calculated by numerical integration based
on a digital terrain model or by representing the topographic masses by a spherical harmonic expansion. To reduce the computation
time in the former case, the integration over the Earth can be divided into two parts: a spherical cap around the computation
point, called the near zone, and the rest of the world, called the far zone. The latter one can be also represented by a global
spherical harmonic expansion. This can be performed by a Molodenskii-type spectral approach. This article extends the original
approach derived in Novák et al. (J Geod 75(9–10):491–504, 2001), which is restricted to determine the far-zone effects for
Helmert’s second method of condensation for ground gravimetry. Here formulae for the far-zone effects of the global topography
on gravity and geoidal heights for Helmert’s first method of condensation as well as for the Airy-Heiskanen model are presented
and some improvements given. Furthermore, this approach is generalized for determining the far-zone effects at aeroplane altitudes.
Numerical results for a part of the Canadian Rocky Mountains are presented to illustrate the size and distributions of these
effects. 相似文献
13.
14.
R. S. Mather 《Journal of Geodesy》1971,45(1):65-88
Summary The alternative harmonic representations of the disturbing potential, correct to the order of the flattening, are examined
and an example is given where the incorrect use of a spherical harmonic expansion can give rise to fallacious results. The
correct usage of the spherical harmonic expansion for the disturbing potential is given in the solution of the general surface
integral to define the indirect effect in the case of the non-regularised geoid. 相似文献
15.
应用文献 [1 ]推导出的球谐系数与椭球谐系数的转换关系 ,给出了椭球界面下Neumann边值问题的积分解 相似文献
16.
Essam Ghanem 《地球空间信息科学学报》2013,16(1):19-23
The main objective of this study is to improve the geoid by GPS/leveling data in Egypt. Comparisons of the gravimetric geoid with GPS/leveling data have been performed. On the basis of a gravimetric geoid fitted to GPS/leveling by the least square method, a smoothed geoid was obtained. A high-resolution geoid in Egypt was computed with a 2.5′×2.5′ grid by combining the data set of 2600 original point gravity values, 20″×30″ resolution Digital Terrain Model (DTM) grid and the spherical harmonic model EGM96. The method of computation involved the strict evaluation of the Stokes integral with 1D-FFT. The standard deviation of the difference between the gravimetric and the GPS/leveling geoid heights is ±0.47 m. The standard deviation after fitting of the gravimetric geoid to the GPS/leveling points is better than ±13 cm. In the future we will try to improve our geoid results in Egypt by increasing the density of gravimetric coverage. 相似文献
17.
Essam Ghanem 《地球空间信息科学学报》2001,4(1):19-23
1 ＩｎｔｒｏｄｕｃｔｉｏｎＤｉｆｆｅｒｅｎｔｇｅｏｉｄｓｏｌｕｔｉｏｎｓｗｅｒｅｃａｒｒｉｅｄｏｕｔｆｏｒＥ ｇｙｐｔｕｓｉｎｇｈｅｔｅｒｏｇｅｎｅｏｕｓｄａｔａａｎｄｄｉｆｆｅｒｅｎｔｍｅｔｈｏｄｏｌｏｇｉｅｓ (Ｅｌ＿Ｔｏｋｈｅｙ ,1 993) .ＴｈｅｍａｉｎｇｏａｌｏｆｔｈｉｓｐａｐｅｒｉｓｔｏｄｅｔｅｒｍｉｎｅａｍｏｓｔａｃｃｕｒａｔｅｎｅｗｇｅｏｉｄｆｏｒＥｇｙｐｔｔａｋｉｎｇａｄｖａｎｔａｇｅｏｆａｎｅｗｕｐｄａｔｅｄｇｒａｖｉｔｙｄａｔａｂａｓｅ,ｔｈｅｉｎｆｏｒｍａｔｉｏｎｇｉｖｅｎｂｙ… 相似文献
18.
目前,航空重力测量是快速获取陆地和近海区域高精度、高分辨率重力场信息的非常有效的技术手段,向下延拓则是其数据处理中的关键环节,直接影响到测量结果的进一步应用。本文在对传统最小二乘法、改进最小二乘法、Tikhonov正则化法等延拓模型进行数值分析的基础上,根据调和函数的基本特性,提出并建立了Poisson积分迭代法和改进Poisson积分迭代法延拓模型。实测航空和地面重力测量数据的试验结果表明,本文新建的Poisson积分迭代法和改进Poisson积分迭代法延拓模型精度相当,比传统最小二乘法延拓模型精度提高了15.26 mGal,比改进最小二乘法延拓模型精度提高了0.21 mGal,比Tikhonov正则化法延拓模型精度略低0.13 mGal,从而证明了本文所建模型的正确性和有效性。 相似文献
19.
Lars E. Sj?berg 《Journal of Geodesy》1988,62(2):93-101
The spherical harmonic coefficients of the Earth’s gravitational potential are conveniently determined by integration of gravity
data or potential data (derived from satellite altimetry) over a sphere. The major problem of such a method is that the data,
given on the non-spherical surface of the Earth, must be reduced to the sphere.
A new integral formula over the surface of the Earth is derived. With this formula improved first order topographic corrections
to the spherical formulas are obtained. 相似文献
20.
This paper is devoted to the spherical and spheroidal harmonic expansion of the gravitational potential of the topographic masses in the most rigorous way. Such an expansion can be used to compute gravimetric topographic effects for geodetic and geophysical applications. It can also be used to augment a global gravity model to a much higher resolution of the gravitational potential of the topography. A formulation for a spherical harmonic expansion is developed without the spherical approximation. Then, formulas for the spheroidal harmonic expansion are derived. For the latter, Legendre’s functions of the first and second kinds with imaginary variable are expanded in Laurent series. They are then scaled into two real power series of the second eccentricity of the reference ellipsoid. Using these series, formulas for computing the spheroidal harmonic coefficients are reduced to surface harmonic analysis. Two numerical examples are presented. The first is a spherical harmonic expansion to degree and order 2700 by taking advantage of existing software. It demonstrates that rigorous spherical harmonic expansion is possible, but the computed potential on the geoid shows noticeable error pattern at Polar Regions due to the downward continuation from the bounding sphere to the geoid. The second numerical example is the spheroidal expansion to degree and order 180 for the exterior space. The power series of the second eccentricity of the reference ellipsoid is truncated at the eighth order leading to omission errors of 25 nm (RMS) for land areas, with extreme values around 0.5 mm to geoid height. The results show that the ellipsoidal correction is 1.65 m (RMS) over land areas, with maximum value of 13.19 m in the Andes. It shows also that the correction resembles the topography closely, implying that the ellipsoidal correction is rich in all frequencies of the gravity field and not only long wavelength as it is commonly assumed. 相似文献