Accuracy Evaluation of Geoid Heights in the National Control Points of South Korea Using High-Degree Geopotential Model
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Evaluation of Recent Global Geopotential Models Based on GPS/Levelling Data Over Afyonkarahisar (Turkey)
Scientific Research and Essays Vol. 5(5), pp. 484-493, 4 March, 2010 Available online at http://www.academicjournals.org/SRE ISSN 1992-2248 © 2010 Academic Journals Full Length Research Paper Evaluation of recent global geopotential models based on GPS/levelling data over Afyonkarahisar (Turkey) Ibrahim Yilmaz1*, Mustafa Yilmaz2, Mevlüt Güllü1 and Bayram Turgut1 1Department of Geodesy and Photogrammetry, Faculty of Engineering, Kocatepe University of Afyonkarahisar, Ahmet Necdet Sezer Campus Gazlıgöl Yolu, 03200, Afyonkarahisar, Turkey. 2Directorship of Afyonkarahisar, Osmangazi Electricity Distribution Inc., Yuzbası Agah Cd. No: 24, 03200, Afyonkarahisar, Turkey. Accepted 20 January, 2010 This study presents the evaluation of the global geo-potential models EGM96, EIGEN-5C, EGM2008(360) and EGM2008 by comparing model based on geoid heights to the GPS/levelling based on geoid heights over Afyonkarahisar study area in order to find the geopotential model that best fits the study area to be used in a further geoid determination at regional and national scales. The study area consists of 313 control points that belong to the Turkish National Triangulation Network, covering a rough area. The geoid height residuals are investigated by standard deviation value after fitting tilt at discrete points, and height-dependent evaluations have been performed. The evaluation results revealed that EGM2008 fits best to the GPS/levelling based on geoid heights than the other models with significant improvements in the study area. Key words: Geopotential model, GPS/levelling, geoid height, EGM96, EIGEN-5C, EGM2008(360), EGM2008. INTRODUCTION Most geodetic applications like determining the topogra- evaluation studies of EGM2008 have been coordinated phic heights or sea depths require the geoid as a by the joint working group (JWG) between the Inter- corresponding reference surface. -
THE EARTH's GRAVITY OUTLINE the Earth's Gravitational Field
GEOPHYSICS (08/430/0012) THE EARTH'S GRAVITY OUTLINE The Earth's gravitational field 2 Newton's law of gravitation: Fgrav = GMm=r ; Gravitational field = gravitational acceleration g; gravitational potential, equipotential surfaces. g for a non–rotating spherically symmetric Earth; Effects of rotation and ellipticity – variation with latitude, the reference ellipsoid and International Gravity Formula; Effects of elevation and topography, intervening rock, density inhomogeneities, tides. The geoid: equipotential mean–sea–level surface on which g = IGF value. Gravity surveys Measurement: gravity units, gravimeters, survey procedures; the geoid; satellite altimetry. Gravity corrections – latitude, elevation, Bouguer, terrain, drift; Interpretation of gravity anomalies: regional–residual separation; regional variations and deep (crust, mantle) structure; local variations and shallow density anomalies; Examples of Bouguer gravity anomalies. Isostasy Mechanism: level of compensation; Pratt and Airy models; mountain roots; Isostasy and free–air gravity, examples of isostatic balance and isostatic anomalies. Background reading: Fowler §5.1–5.6; Lowrie §2.2–2.6; Kearey & Vine §2.11. GEOPHYSICS (08/430/0012) THE EARTH'S GRAVITY FIELD Newton's law of gravitation is: ¯ GMm F = r2 11 2 2 1 3 2 where the Gravitational Constant G = 6:673 10− Nm kg− (kg− m s− ). ¢ The field strength of the Earth's gravitational field is defined as the gravitational force acting on unit mass. From Newton's third¯ law of mechanics, F = ma, it follows that gravitational force per unit mass = gravitational acceleration g. g is approximately 9:8m/s2 at the surface of the Earth. A related concept is gravitational potential: the gravitational potential V at a point P is the work done against gravity in ¯ P bringing unit mass from infinity to P. -
The Evolution of Earth Gravitational Models Used in Astrodynamics
JEROME R. VETTER THE EVOLUTION OF EARTH GRAVITATIONAL MODELS USED IN ASTRODYNAMICS Earth gravitational models derived from the earliest ground-based tracking systems used for Sputnik and the Transit Navy Navigation Satellite System have evolved to models that use data from the Joint United States-French Ocean Topography Experiment Satellite (Topex/Poseidon) and the Global Positioning System of satellites. This article summarizes the history of the tracking and instrumentation systems used, discusses the limitations and constraints of these systems, and reviews past and current techniques for estimating gravity and processing large batches of diverse data types. Current models continue to be improved; the latest model improvements and plans for future systems are discussed. Contemporary gravitational models used within the astrodynamics community are described, and their performance is compared numerically. The use of these models for solid Earth geophysics, space geophysics, oceanography, geology, and related Earth science disciplines becomes particularly attractive as the statistical confidence of the models improves and as the models are validated over certain spatial resolutions of the geodetic spectrum. INTRODUCTION Before the development of satellite technology, the Earth orbit. Of these, five were still orbiting the Earth techniques used to observe the Earth's gravitational field when the satellites of the Transit Navy Navigational Sat were restricted to terrestrial gravimetry. Measurements of ellite System (NNSS) were launched starting in 1960. The gravity were adequate only over sparse areas of the Sputniks were all launched into near-critical orbit incli world. Moreover, because gravity profiles over the nations of about 65°. (The critical inclination is defined oceans were inadequate, the gravity field could not be as that inclination, 1= 63 °26', where gravitational pertur meaningfully estimated. -
A Hierarchy of Models, from Planetary to Mesoscale, Within a Single
A hierarchy of models, from planetary to mesoscale, within a single switchable numerical framework Nigel Wood, Andy White and Andrew Staniforth Dynamics Research, Met Office © Crown copyright Met Office Outline of the talk • Overview of Met Office’s Unified Model • Spherical Geopotential Approximation • Relaxing that approximation • A method of implementation • Alternative view of Shallow-Atmosphere Approximation • Application to departure points © Crown copyright Met Office Met Office’s Unified Model Unified Model (UM) in that single model for: Operational forecasts at ¾Mesoscale (resolution approx. 12km → 4km → 1km) ¾Global scale (resolution approx. 25km) Global and regional climate predictions (resolution approx. 100km, run for 10-100 years) + Research mode (1km - 10m) and single column model 20 years old this year © Crown copyright Met Office Timescales & applications © Crown copyright Met Office © Crown copyright Met Office UKV Domain 4x4 1.5x4 4x4 4x1.5 1.5x1.5 4x1.5 4x4 1.5x4 4x4 Variable 744(622) x 928( 810) points zone © Crown copyright Met Office The ‘Morpeth Flood’, 06/09/2008 1.5 km L70 Prototype UKV From 15 UTC 05/09 12 km 0600 UTC © Crown copyright Met Office 2009: Clark et al, Morpeth Flood UKV 4-20hr forecast 1.5km gridlength UK radar network convection permitting model © Crown copyright Met Office © Crown copyright Met Office © Crown copyright Met Office The underlying equations... c Crown Copyright Met Office © Crown copyright Met Office Traditional Spherically Based Equations Dru uv tan φ cpdθv ∂Π uw u − − (2Ω sin -
Geophysical Journal International
Geophysical Journal International Geophys. J. Int. (2015) 203, 1773–1786 doi: 10.1093/gji/ggv392 GJI Gravity, geodesy and tides GRACE time-variable gravity field recovery using an improved energy balance approach Kun Shang,1 Junyi Guo,1 C.K. Shum,1,2 Chunli Dai1 and Jia Luo3 1Division of Geodetic Science, School of Earth Sciences, The Ohio State University, 125 S. Oval Mall, Columbus, OH 43210, USA. E-mail: [email protected] 2Institute of Geodesy & Geophysics, Chinese Academy of Sciences, Wuhan, China 3School of Geodesy and Geomatics, Wuhan University, 129 Luoyu Road, Wuhan 430079, China Accepted 2015 September 14. Received 2015 September 12; in original form 2015 March 19 Downloaded from SUMMARY A new approach based on energy conservation principle for satellite gravimetry mission has been developed and yields more accurate estimation of in situ geopotential difference observ- ables using K-band ranging (KBR) measurements from the Gravity Recovery and Climate Experiment (GRACE) twin-satellite mission. This new approach preserves more gravity in- http://gji.oxfordjournals.org/ formation sensed by KBR range-rate measurements and reduces orbit error as compared to previous energy balance methods. Results from analysis of 11 yr of GRACE data indicated that the resulting geopotential difference estimates agree well with predicted values from of- ficial Level 2 solutions: with much higher correlation at 0.9, as compared to 0.5–0.8 reported by previous published energy balance studies. We demonstrate that our approach produced a comparable time-variable gravity solution with the Level 2 solutions. The regional GRACE temporal gravity solutions over Greenland reveals that a substantially higher temporal resolu- at Ohio State University Libraries on December 20, 2016 tion is achievable at 10-d sampling as compared to the official monthly solutions, but without the compromise of spatial resolution, nor the need to use regularization or post-processing. -
The Joint Gravity Model 3
Journal of Geophysical Research Accepted for publication, 1996 The Joint Gravity Model 3 B. D. Tapley, M. M. Watkins,1 J. C. Ries, G. W. Davis,2 R. J. Eanes, S. R. Poole, H. J. Rim, B. E. Schutz, and C. K. Shum Center for Space Research, University of Texas at Austin R. S. Nerem,3 F. J. Lerch, and J. A. Marshall Space Geodesy Branch, NASA Goddard Space Flight Center, Greenbelt, Maryland S. M. Klosko, N. K. Pavlis, and R. G. Williamson Hughes STX Corporation, Lanham, Maryland Abstract. An improved Earth geopotential model, complete to spherical harmonic degree and order 70, has been determined by combining the Joint Gravity Model 1 (JGM 1) geopotential coef®cients, and their associated error covariance, with new information from SLR, DORIS, and GPS tracking of TOPEX/Poseidon, laser tracking of LAGEOS 1, LAGEOS 2, and Stella, and additional DORIS tracking of SPOT 2. The resulting ®eld, JGM 3, which has been adopted for the TOPEX/Poseidon altimeter data rerelease, yields improved orbit accuracies as demonstrated by better ®ts to withheld tracking data and substantially reduced geographically correlated orbit error. Methods for analyzing the performance of the gravity ®eld using high-precision tracking station positioning were applied. Geodetic results, including station coordinates and Earth orientation parameters, are signi®cantly improved with the JGM 3 model. Sea surface topography solutions from TOPEX/Poseidon altimetry indicate that the ocean geoid has been improved. Subset solutions performed by withholding either the GPS data or the SLR/DORIS data were computed to demonstrate the effect of these particular data sets on the gravity model used for TOPEX/Poseidon orbit determination. -
Vertical Structure
ESCI 341 – Atmospheric Thermodynamics Lesson 7 – Vertical Structure References: An Introduction to Dynamic Meteorology, Holton Introduction to Theoretical Meteorology, Hess Synoptic-dynamic Meteorology in Midlatitudes, Vol. 1, Bluestein ‘An example of uncertainty in sea level pressure reduction’, P.M. Pauley, Mon. Wea. Rev., 13, 1998, pp. 833-850 GEOPOTENTIAL l The acceleration due to gravity is not constant. It varies from place to place, with the largest variation due to latitude. o What we call gravity is the combination of the gravitational acceleration and the centrifugal acceleration from the Earth’s rotation. o Gravity at the North Pole is approximately 9.83 m/s2, while at the Equator it is about 9.78 m/s2. l Though small, the variation in gravity must be accounted for. We do this via the concept of geopotential. l Geopotential is essentially the potential energy per unit mass. l A surface of constant geopotential represents a surface along which all objects of the same mass have the same potential energy. l If gravity were constant, a geopotential surface would lie at a constant altitude. Since gravity is not constant, a geopotential surface will have varying altitude. l Geopotential is defined as z F º ò gdz, (1) 0 or in differential form as dF = gdz. l Geopotential height is defined as F 1 Z Zº=ò gdZ (2) gg000 2 where g0 is a constant called standard gravity, and has a value of 9.80665 m/s . o Geopotential height is expressed in geopotential meters, abbreviated as gpm. l If the change in gravity with height is ignored, geopotential height and geometric height are related via g Z = z. -
Spline Representations of Functions on a Sphere for Geopotential Modeling
Spline Representations of Functions on a Sphere for Geopotential Modeling by Christopher Jekeli Report No. 475 Geodetic and GeoInformation Science Department of Civil and Environmental Engineering and Geodetic Science The Ohio State University Columbus, Ohio 43210-1275 March 2005 Spline Representations of Functions on a Sphere for Geopotential Modeling Final Technical Report Christopher Jekeli Laboratory for Space Geodesy and Remote Sensing Research Department of Civil and Environmental Engineering and Geodetic Science Ohio State University Prepared Under Contract NMA302-02-C-0002 National Geospatial-Intelligence Agency November 2004 Preface This report was prepared with support from the National Geospatial-Intelligence Agency under contract NMA302-02-C-0002 and serves as the final technical report for this project. ii Abstract Three types of spherical splines are presented as developed in the recent literature on constructive approximation, with a particular view towards global (and local) geopotential modeling. These are the tensor-product splines formed from polynomial and trigonometric B-splines, the spherical splines constructed from radial basis functions, and the spherical splines based on homogeneous Bernstein-Bézier (BB) polynomials. The spline representation, in general, may be considered as a suitable alternative to the usual spherical harmonic model, where the essential benefit is the local support of the spline basis functions, as opposed to the global support of the spherical harmonics. Within this group of splines each has distinguishing characteristics that affect their utility for modeling the Earth’s gravitational field. Tensor-product splines are most straightforwardly constructed, but require data on a grid of latitude and longitude coordinate lines. The radial-basis splines resemble the collocation solution in physical geodesy and are most easily extended to three-dimensional space according to potential theory. -
ICGEM – 15 Years of Successful Collection and Distribution of Global Gravitational Models, Associated Services and Future Plans
ICGEM – 15 years of successful collection and distribution of global gravitational models, associated services and future plans E. Sinem Ince1, Franz Barthelmes1, Sven Reißland1, Kirsten Elger2, Christoph Förste1, Frank 5 Flechtner1,4, and Harald Schuh3,4 1Section 1.2: Global Geomonitoring and Gravity Field, GFZ German Research Centre for Geosciences, Potsdam, Germany 2Library and Information Services, GFZ German Research Centre for Geosciences, Potsdam, Germany 3Section 1.1: Space Geodetic Techniques, GFZ German Research Centre for Geosciences, Potsdam, Germany 10 4Department of Geodesy and Geoinformation Science, Technical University of Berlin, Berlin, Germany Correspondence to: E. Sinem Ince ([email protected]) Abstract. The International Centre for Global Earth Models (ICGEM, http://icgem.gfz-potsdam.de/) hosted at the GFZ German Research Centre for Geosciences (GFZ) is one of the five Services coordinated by the International Gravity Field Service (IGFS) of the International Association of Geodesy (IAG). The goal of the ICGEM Service is to provide the 15 scientific community with a state of the art archive of static and temporal global gravity field models of the Earth, and develop and operate interactive calculation and visualisation services of gravity field functionals on user defined grids or at a list of particular points via its website. ICGEM offers the largest collection of global gravity field models, including those from the 1960s to the 1990s, as well as the most recent ones that have been developed using data from dedicated satellite gravity missions, CHAMP, GRACE, and GOCE, advanced processing methodologies and additional data sources such as 20 satellite altimetry and terrestrial gravity. -
6. the Gravity Field
6. The Gravity Field Ge 163 4/11/14- Outline • Spherical Harmonics • Gravitational potential in spherical harmonics • Potential in terms of moments of inertia • The Geopotential • Flattening and the excess bulge of the earth • The geoid and geoid height • Non-hydrostatic geoid • Geoid over slabs • Geoid correlation with hot-spots & Ancient Plate boundaries • GRACE: Gravity Recovery And Climate Experiment Spherical harmonics ultimately stem from the solution of Laplace’s equation. Find a solution of Laplace’s equation in a spherical coordinate system. ∇2 f = 0 The Laplacian operator can be written as 2 1 ∂ ⎛ 2 ∂f ⎞ 1 ∂ ⎛ ∂f ⎞ 1 ∂ f 2 ⎜ r ⎟ + 2 ⎜ sinθ ⎟ + 2 2 2 = 0 r ∂r ⎝ ∂r ⎠ r sinθ ∂θ ⎝ ∂θ ⎠ r sin θ ∂λ r is radius θ is colatitude λ Is longitude One way to solve the Laplacian in spherical coordinates is through separation of variables f = R(r)P(θ)L(λ) To demonstrate the form of the spherical harmonic, one can take a simple form of R(r ). This is not the only one which solves the equation, but it is sufficient to demonstrate the form of the solution. Guess R(r) = rl f = rl P(θ)L(λ) 1 ∂ ⎛ ∂P(θ)⎞ 1 ∂2 L(λ) l(l + 1) + ⎜ sinθ ⎟ + 2 2 = 0 sinθP(θ) ∂θ ⎝ ∂θ ⎠ sin θL(λ) ∂λ This is the only place where λ appears, consequently it must be equal to a constant 1 ∂2 L(λ) = constant = −m2 m is an integer L(λ) ∂λ 2 L(λ) = Am cos mλ + Bm sin mλ This becomes: 1 ∂ ⎛ ∂P(θ)⎞ ⎡ m2 ⎤ ⎜ sinθ ⎟ + ⎢l(l + 1) − 2 ⎥ P(θ) = 0 sinθ ∂θ ⎝ ∂θ ⎠ ⎣ sin θ ⎦ This equation is known as Legendre’s Associated equation The solution of P(θ) are polynomials in cosθ, involving the integers l and m. -
Preparation of Papers for AIAA Technical Conferences
Gravity Modeling for Variable Fidelity Environments Michael M. Madden* NASA, Hampton, VA, 23681 Aerospace simulations can model worlds, such as the Earth, with differing levels of fidel- ity. The simulation may represent the world as a plane, a sphere, an ellipsoid, or a high- order closed surface. The world may or may not rotate. The user may select lower fidelity models based on computational limits, a need for simplified analysis, or comparison to other data. However, the user will also wish to retain a close semblance of behavior to the real world. The effects of gravity on objects are an important component of modeling real-world behavior. Engineers generally equate the term gravity with the observed free-fall accelera- tion. However, free-fall acceleration is not equal to all observers. To observers on the sur- face of a rotating world, free-fall acceleration is the sum of gravitational attraction and the centrifugal acceleration due to the world’s rotation. On the other hand, free-fall accelera- tion equals gravitational attraction to an observer in inertial space. Surface-observed simu- lations (e.g. aircraft), which use non-rotating world models, may choose to model observed free fall acceleration as the “gravity” term; such a model actually combines gravitational at- traction with centrifugal acceleration due to the Earth’s rotation. However, this modeling choice invites confusion as one evolves the simulation to higher fidelity world models or adds inertial observers. Care must be taken to model gravity in concert with the world model to avoid denigrating the fidelity of modeling observed free fall. -
An Oceanographer's Guide to GOCE and the Geoid
An Oceanographer’s Guide to GOCE and the Geoid C. W. Hughes, R. J. Bingham To cite this version: C. W. Hughes, R. J. Bingham. An Oceanographer’s Guide to GOCE and the Geoid. Ocean Science, European Geosciences Union, 2008, 4 (1), pp.15-29. hal-00298352 HAL Id: hal-00298352 https://hal.archives-ouvertes.fr/hal-00298352 Submitted on 24 Jan 2008 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Ocean Sci., 4, 15–29, 2008 www.ocean-sci.net/4/15/2008/ Ocean Science © Author(s) 2008. This work is licensed under a Creative Commons License. An Oceanographer’s Guide to GOCE and the Geoid C. W. Hughes and R. J. Bingham Proudman Oceanographic Laboratory, 6 Brownlow St., Liverpool L3 5DA, UK Received: 5 September 2006 – Published in Ocean Sci. Discuss.: 20 September 2006 Revised: 28 November 2007 – Accepted: 14 December 2007 – Published: 24 January 2008 Abstract. A review is given of the geodetic concepts nec- essary to understand the time dependent gravity field and its essary for oceanographers to make use of satellite gravity relationship to mass movements in the earth system.