Preliminary Estimation and Validation of Polar Motion Excitation from Different Types of the GRACE and GRACE Follow-On Missions Data
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Detection of Caves by Gravimetry
Detection of Caves by Gravimetry By HAnlUi'DO J. Cmco1) lVi/h plates 18 (1)-21 (4) Illtroduction A growing interest in locating caves - largely among non-speleolo- gists - has developed within the last decade, arising from industrial or military needs, such as: (1) analyzing subsUl'face characteristics for building sites or highway projects in karst areas; (2) locating shallow caves under airport runways constructed on karst terrain covered by a thin residual soil; and (3) finding strategic shelters of tactical significance. As a result, geologists and geophysicists have been experimenting with the possibility of applying standard geophysical methods toward void detection at shallow depths. Pioneering work along this line was accomplishecl by the U.S. Geological Survey illilitary Geology teams dUl'ing World War II on Okinawan airfields. Nicol (1951) reported that the residual soil covel' of these runways frequently indicated subsi- dence due to the collapse of the rooves of caves in an underlying coralline-limestone formation (partially detected by seismic methods). In spite of the wide application of geophysics to exploration, not much has been published regarding subsUl'face interpretation of ground conditions within the upper 50 feet of the earth's surface. Recently, however, Homberg (1962) and Colley (1962) did report some encoUl'ag- ing data using the gravity technique for void detection. This led to the present field study into the practical means of how this complex method can be simplified, and to a use-and-limitations appraisal of gravimetric techniques for speleologic research. Principles all(1 Correctiolls The fundamentals of gravimetry are based on the fact that natUl'al 01' artificial voids within the earth's sUl'face - which are filled with ail' 3 (negligible density) 01' water (density about 1 gmjcm ) - have a remark- able density contrast with the sUl'roun<ling rocks (density 2.0 to 1) 4609 Keswick Hoad, Baltimore 10, Maryland, U.S.A. -
Airborne Geoid Determination
LETTER Earth Planets Space, 52, 863–866, 2000 Airborne geoid determination R. Forsberg1, A. Olesen1, L. Bastos2, A. Gidskehaug3,U.Meyer4∗, and L. Timmen5 1KMS, Geodynamics Department, Rentemestervej 8, 2400 Copenhagen NV, Denmark 2Astronomical Observatory, University of Porto, Portugal 3Institute of Solid Earth Physics, University of Bergen, Norway 4Alfred Wegener Institute, Bremerhaven, Germany 5Geo Forschungs Zentrum, Potsdam, Germany (Received January 17, 2000; Revised August 18, 2000; Accepted August 18, 2000) Airborne geoid mapping techniques may provide the opportunity to improve the geoid over vast areas of the Earth, such as polar areas, tropical jungles and mountainous areas, and provide an accurate “seam-less” geoid model across most coastal regions. Determination of the geoid by airborne methods relies on the development of airborne gravimetry, which in turn is dependent on developments in kinematic GPS. Routine accuracy of airborne gravimetry are now at the 2 mGal level, which may translate into 5–10 cm geoid accuracy on regional scales. The error behaviour of airborne gravimetry is well-suited for geoid determination, with high-frequency survey and downward continuation noise being offset by the low-pass gravity to geoid filtering operation. In the paper the basic principles of airborne geoid determination are outlined, and examples of results of recent airborne gravity and geoid surveys in the North Sea and Greenland are given. 1. Introduction the sea-surface (H) by airborne altimetry. This allows— Precise geoid determination has in recent years been facil- in principle—the determination of the dynamic sea-surface itated through the progress in airborne gravimetry. The first topography (ζ) through the equation large-scale aerogravity experiment was the airborne gravity survey of Greenland 1991–92 (Brozena, 1991). -
Resolving Geophysical Signals by Terrestrial Gravimetry: a Time Domain Assessment of the Correction-Induced Uncertainty
Originally published as: Mikolaj, M., Reich, M., Güntner, A. (2019): Resolving Geophysical Signals by Terrestrial Gravimetry: A Time Domain Assessment of the Correction-Induced Uncertainty. - Journal of Geophysical Research, 124, 2, pp. 2153—2165. DOI: http://doi.org/10.1029/2018JB016682 RESEARCH ARTICLE Resolving Geophysical Signals by Terrestrial Gravimetry: 10.1029/2018JB016682 A Time Domain Assessment of the Correction-Induced Key Points: Uncertainty • Global-scale uncertainty assessment of tidal, oceanic, large-scale 1 1 1,2 hydrological, and atmospheric M. Mikolaj , M. Reich , and A. Güntner corrections for terrestrial gravimetry • Resolving subtle gravity signals in the 1Section Hydrology, GFZ German Research Centre for Geosciences, Potsdam, Germany, 2Institute of Environmental order of few nanometers per square Science and Geography, University of Potsdam, Potsdam, Germany second is challenged by the statistical uncertainty of correction models • Uncertainty computed for selected periods varies significantly Abstract Terrestrial gravimetry is increasingly used to monitor mass transport processes in with latitude and altitude of the geophysics boosted by the ongoing technological development of instruments. Resolving a particular gravimeter phenomenon of interest, however, requires a set of gravity corrections of which the uncertainties have not been addressed up to now. In this study, we quantify the time domain uncertainty of tide, global Supporting Information: atmospheric, large-scale hydrological, and nontidal ocean loading corrections. The uncertainty is • Supporting Information S1 assessed by comparing the majority of available global models for a suite of sites worldwide. The average uncertainty expressed as root-mean-square error equals 5.1 nm/s2, discounting local hydrology or air Correspondence to: pressure. The correction-induced uncertainty of gravity changes over various time periods of interest M. -
Macroscopic Superpositions and Gravimetry with Quantum Magnetomechanics Received: 07 July 2016 Mattias T
www.nature.com/scientificreports OPEN Macroscopic superpositions and gravimetry with quantum magnetomechanics Received: 07 July 2016 Mattias T. Johnsson, Gavin K. Brennen & Jason Twamley Accepted: 24 October 2016 Precision measurements of gravity can provide tests of fundamental physics and are of broad Published: 21 November 2016 practical interest for metrology. We propose a scheme for absolute gravimetry using a quantum magnetomechanical system consisting of a magnetically trapped superconducting resonator whose motion is controlled and measured by a nearby RF-SQUID or flux qubit. By driving the mechanical massive resonator to be in a macroscopic superposition of two different heights our we predict that our interferometry protocol could, subject to systematic errors, achieve a gravimetric sensitivity of Δg/g ~ 2.2 × 10−10 Hz−1/2, with a spatial resolution of a few nanometres. This sensitivity and spatial resolution exceeds the precision of current state of the art atom-interferometric and corner-cube gravimeters by more than an order of magnitude, and unlike classical superconducting interferometers produces an absolute rather than relative measurement of gravity. In addition, our scheme takes measurements at ~10 kHz, a region where the ambient vibrational noise spectrum is heavily suppressed compared the ~10 Hz region relevant for current cold atom gravimeters. Gravimetry is the measurement of the local acceleration due to gravity on a test body. As gravity is an infinite range force that cannot be shielded against, it provides a useful probe for a variety of effects over a wide range of distances. Given a theory of gravity, gravimetry provides information about local mass distribution or, given a known, local mass distribution, it provides information that can be used test theories of gravity. -
Pendulum MEMS Gravimeters for Semi-Absolute Gravimetry
EGU2020-1244 https://doi.org/10.5194/egusphere-egu2020-1244 EGU General Assembly 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Pendulum MEMS gravimeters for semi-absolute gravimetry Richard Middlemiss1, Giles Hammond2, Richard Walker2, and Abhinav Prasad2 1University of Glasgow, James Watt School of Engineering, Glasgow, United Kingdom of Great Britain and Northern Ireland ([email protected]) 2University of Glasgow, Institute for Gravitational Research, Glasgow, United Kingdom of Great Britain and Northern Ireland By measuring tiny variations in the Earth’s gravitational acceleration, g, one can infer density variations beneath the ground. Since magmatic systems contain rock of differing density, changes in gravity over time can tell us when/where magma is moving. Traditional gravity sensors (gravimeters) were costly and heavy, but with the advent of the technology used to make mobile phone accelerometers (MEMS – Microelectromechanical-systems), this is changing. At Glasgow University we have already developed the first MEMS gravity sensor and we are now working with several other European institutions to make a network of gravity sensors around Mt Etna – NEWTON-g. It will be the first multi-pixel gravity imager – enabling unprecedented resolution of Etna’s plumbing system. While this work is ongoing, a second generation of MEMS gravity sensor is now under development. The first-generation sensor comprises a mass on a spring, which moves in response to changing values of g. This, however, can only ever be used to measure changes in gravity, which means it can be difficult to tell the difference between a geophysical signal and instrumental drift. -
True Polar Wander: Linking Deep and Shallow Geodynamics to Hydro- and Bio-Spheric Hypotheses T
True Polar Wander: linking Deep and Shallow Geodynamics to Hydro- and Bio-Spheric Hypotheses T. D. Raub, Yale University, New Haven, CT, USA J. L. Kirschvink, California Institute of Technology, Pasadena, CA, USA D. A. D. Evans, Yale University, New Haven, CT, USA © 2007 Elsevier SV. All rights reserved. 5.14.1 Planetary Moment of Inertia and the Spin-Axis 565 5.14.2 Apparent Polar Wander (APW) = Plate motion +TPW 566 5.14.2.1 Different Information in Different Reference Frames 566 5.14.2.2 Type 0' TPW: Mass Redistribution at Clock to Millenial Timescales, of Inconsistent Sense 567 5.14.2.3 Type I TPW: Slow/Prolonged TPW 567 5.14.2.4 Type II TPW: Fast/Multiple/Oscillatory TPW: A Distinct Flavor of Inertial Interchange 569 5.14.2.5 Hypothesized Rapid or Prolonged TPW: Late Paleozoic-Mesozoic 569 5.14.2.6 Hypothesized Rapid or Prolonged TPW: 'Cryogenian'-Ediacaran-Cambrian-Early Paleozoic 571 5.14.2.7 Hypothesized Rapid or Prolonged TPW: Archean to Mesoproterozoic 572 5.14.3 Geodynamic and Geologic Effects and Inferences 572 5.14.3.1 Precision of TPW Magnitude and Rate Estimation 572 5.14.3.2 Physical Oceanographic Effects: Sea Level and Circulation 574 5.14.3.3 Chemical Oceanographic Effects: Carbon Oxidation and Burial 576 5..14.4 Critical Testing of Cryogenian-Cambrian TPW 579 5.14A1 Ediacaran-Cambrian TPW: 'Spinner Diagrams' in the TPW Reference Frame 579 5.14.4.2 Proof of Concept: Independent Reconstruction of Gondwanaland Using Spinner Diagrams 581 5.14.5 Summary: Major Unresolved Issues and Future Work 585 References 586 5.14.1 Planetary Moment of Inertia location ofEarth's daily rotation axis and/or by fluc and the Spin-Axis tuations in the spin rate ('length of day' anomalies). -
Earth Orientation Parameters from VLBI Determined with a Kalman Filter
Originally published as: Karbon, M., Soja, B., Nilsson, T., Deng, Z., Heinkelmann, R., Schuh, H. (2017): Earth orientation parameters from VLBI determined with a Kalman filter. ‐ Geodesy and Geodynamics, 8, 6, pp. 396— 407. DOI: http://doi.org/10.1016/j.geog.2017.05.006 Geodesy and Geodynamics 8 (2017) 396e407 Contents lists available at ScienceDirect Geodesy and Geodynamics journal homepages: www.keaipublishing.com/en/journals/geog; http://www.jgg09.com/jweb_ddcl_en/EN/volumn/home.shtml Earth orientation parameters from VLBI determined with a Kalman filter * Maria Karbon a, , Benedikt Soja b, Tobias Nilsson a, Zhiguo Deng a, Robert Heinkelmann a, Harald Schuh a, c a GFZ German Research Centre for Geosciences, Telegrafenberg A17, Potsdam, Germany b Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA c Technical University of Berlin, Strabe des 17. Juni 135, Berlin, Germany article info abstract Article history: This paper introduces the reader to our Kalman filter developed for geodetic VLBI (very long baseline Received 24 November 2016 interferometry) data analysis. The focus lies on the EOP (Earth Orientation Parameter) determination Received in revised form based on the Continuous VLBI Campaign 2014 (CONT14) data, but also earlier CONT campaigns are 23 May 2017 analyzed. For validation and comparison purposes we use EOP determined with the classical LSM Accepted 24 May 2017 (least squares method) estimated from the same VLBI data set as the Kalman solution with a daily Available online 6 September 2017 resolution. To gain higher resolved EOP from LSM we run solutions which yield hourly estimates for polar motion and dUT1 ¼ Universal Time (UT1) e Coordinated Universal Time (UTC). -
Gravimetric Geoid Modelling Over Peninsular Malaysia Using Two Different Gridding Approaches for Combining Free Air Anomaly
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XLII-4/W16, 2019 6th International Conference on Geomatics and Geospatial Technology (GGT 2019), 1–3 October 2019, Kuala Lumpur, Malaysia GRAVIMETRIC GEOID MODELLING OVER PENINSULAR MALAYSIA USING TWO DIFFERENT GRIDDING APPROACHES FOR COMBINING FREE AIR ANOMALY M F Pa’suya 1,2* ,A H M Din 2,3, J. C. McCubbine4 ,A.H.Omar2 , Z. M. Amin 3 and N.A.Z.Yahaya2 1Center of Studies for Surveying Science and Geomatics, Faculty of Architecture, Planning & Surveying, Universiti Teknologi MARA, Perlis, Arau Campus, 02600 Arau, Perlis - [email protected] 2 Geomatics Innovation Research Group (GNG) , 3Geoscience and Digital Earth Centre (INSTEG), Faculty of Built Environment and Surveying, Universiti Teknologi Malaysia, 81310 Johor Bahru, Johor, Malaysia- [email protected] 4 Geodesy Section, Community Safety and Earth Monitoring Division, Geoscience Australia, GPO Box 378, Canberra, ACT 2601, Australia- [email protected] KEY WORDS: LSMSA, KTH method ,gravimetric geoid, Peninsular Malaysia ABSTRACT: We investigate the use of the KTH Method to compute gravimetric geoid models of Malaysian Peninsular and the effect of two differing strategies to combine and interpolate terrestrial, marine DTU17 free air gravity anomaly data at regular grid nodes. Gravimetric geoid models were produced for both free air anomaly grids using the GOCE-only geopotential model GGM GO_CONS_GCF_2_SPW_R4 as the long wavelength reference signal and high-resolution TanDEM-X global digital terrain model. The geoid models were analyzed to assess how the different gridding strategies impact the gravimetric geoid over Malaysian Peninsular by comparing themto 172 GNSS-levelling derived geoid undulations. -
Gravity Measurements in Bolivia and Their Implications for the Tectonic Development of the Central Andean Plateau
Gravity Measurements in Bolivia and their Implications for the Tectonic Development of the Central Andean Plateau DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Kevin M. Ahlgren Graduate Program in Geodetic Science The Ohio State University 2015 Dissertation Committee: Michael Bevis, Advisor Alan Saalfeld Ralph von Frese Copyright by Kevin M. Ahlgren 2015 ABSTRACT A geodetic network of gravity stations in Bolivia was established, reduced, adjusted, and analyzed. This network consists of more than 1300 relative stations with estimated precisions of less than ±0.15 mGal. The network is supported and adjusted using 15 absolute gravity stations. The motivation for observing a completely new and large gravity network in Bolivia is to contribute to the global geopotential model (GGM), which will eventually succeed EGM2008, to provide Bolivia with a much-improved height system, and to use these results to place new geophysical constraints on geodynamic models of the Central Andes. The Central Andes comprise an area of South America associated with a widening of the Andean mountain belt. The evolution of this portion of the range is not completely understood. Traditionally, models with large amounts of steady crustal shortening and thickening over a period of time from 30 Ma - 10 Ma have been hypothesized. Recently, an alternative hypothesis involving a rapid rise of the Central Andes between 10 - 6.8 Ma has been proposed. A tectonic model of this rapid rise hypothesis is developed using locally-compensated isostatic assumptions and delamination of a dense layer of eclogite in the lithospheric mantle. -
Symposium 2B: Earth's Time-Variable Gravity Field
Symposium 2b: Earth’s time-variable gravity field Organizer: Adrian Jäggi (Switzerland) President Commission 2 Co-organizers: Frank Flechtner (Germany) Chair Sub-Commission 2.3 Wei Feng (China) Chair Sub-Commission 2.6 Srinivas Bettadpur (USA) Organiser of GGHS 2020 (resp. GGHS 2022) Abstract Earth’s time-variable gravity field is related to the mass transport and the physical processes within Earth’s system (including the atmosphere, oceans, hydrology and cryosphere), such as melting of ice sheets and glaciers, ocean circulation and sea level variations, hydrological cycle, post-glacial rebound and earthquake-induced gravity change. Nowadays, satellite gravimetry missions, particularly the Gravity Recovery and Climate Experiment (GRACE) and GRACE Follow-On, showed great success to estimate the time-varying gravity field with unprecedented accuracy and resolution, which has been widely used to investigate mass flux within the ocean-land water cycle and Earth’s system coupling as well as responses to climate change together with complimentary data from altimetry, GNSS, and InSAR. This interdisciplinary symposium solicits contributions on (1) time-varying gravity field estimation and improvement from satellite gravimetry missions and combination synergies, (2) mass transport in the Earth system and responses to climate change, and (3) status and simulated results of future time-varying gravity field missions. Symposium 2b: Session 1. Analysis Techniques Convener: Adrian Jäggi, University of Bern, Switzerland, [email protected] Co-convener: Andreas Kvas, Graz University of Technology, Austria, [email protected] Yunzhong Shen (China) Abstract The recovery of Earth’s time variable gravity field from satellite data, especially from the Gravity Recovery and Climate Experiment (GRACE) and from GRACE Follow-On (GRACE-FO), has enabled the study of mass transport on a global scale. -
Constraining Ceres' Interior from Its Rotational Motion
A&A 535, A43 (2011) Astronomy DOI: 10.1051/0004-6361/201116563 & c ESO 2011 Astrophysics Constraining Ceres’ interior from its rotational motion N. Rambaux1,2, J. Castillo-Rogez3, V. Dehant4, and P. Kuchynka2,3 1 Université Pierre et Marie Curie, UPMC–Paris 06, France e-mail: [nicolas.rambaux;kuchynka]@imcce.fr 2 IMCCE, Observatoire de Paris, CNRS UMR 8028, 77 avenue Denfert-Rochereau, 75014 Paris, France 3 Jet Propulsion Laboratory, Caltech, Pasadena, USA e-mail: [email protected] 4 Royal Observatory of Belgium, 3 avenue Circulaire, 1180 Brussels, Belgium Received 24 January 2011 / Accepted 14 July 2011 ABSTRACT Context. Ceres is the most massive body of the asteroid belt and contains about 25 wt.% (weight percent) of water. Understanding its thermal evolution and assessing its current state are major goals of the Dawn mission. Constraints on its internal structure can be inferred from various types of observations. In particular, detailed knowledge of the rotational motion can help constrain the mass distribution inside the body, which in turn can lead to information about its geophysical history. Aims. We investigate the signature of internal processes on Ceres rotational motion and discuss future measurements that can possibly be performed by the spacecraft Dawn and will help to constrain Ceres’ internal structure. Methods. We compute the polar motion, precession-nutation, and length-of-day variations. We estimate the amplitudes of the rigid and non-rigid responses for these various motions for models of Ceres’ interior constrained by shape data and surface properties. Results. As a general result, the amplitudes of oscillations in the rotation appear to be small, and their determination from spaceborne techniques will be challenging. -
Present True Polar Wander in the Frame of the Geotectonic Reference System
1661-8726/08/030629-8 Swiss J. Geosci. 101 (2008) 629–636 DOI 10.1007/s00015-008-1284-y Birkhäuser Verlag, Basel, 2008 Present true polar wander in the frame of the Geotectonic Reference System NAZARIO PAVONI Key words: Geotectonic Reference System, polar wander, geodynamics, geotectonic bipolarity ABSTRACT The Mesozoic-Cenozoic evolution of the Earth’s lithosphere reveals a funda- mA which are responsible for the two geoid highs results in the long-standing mental hemispherical symmetry inherent in global tectonics. The symmetry stability of location of the geotectonic axis PA. The Earth’s rotation axis is is documented by the concurrent regular growth of the Pacific and African oriented perpendicularly to the PA axis. Owing to the extraordinary stabil- plates over the past 180 million years, and by the antipodal position of the two ity of the geotectonic axis, any change of orientation of the rotation axis, e.g. plates. The plates are centered on the equator, where center P of the Pacific induced by post-glacial rebound, occurs in such a way that the axis remains plate is located at 170° W/0° N, and center A of the African plate at 10° E/0° N. in the equatorial plane of the geotectonic system, i.e. in the 80° W/100° E P and A define a system of spherical coordinates, the Geotectonic Reference meridional plane. Observed present polar wander is directed towards 80° W System GRS, which shows a distinct relation to Cenozoic global tectonics. P (79.2 ± 0.2° W). This indicates that the present true polar wander is directed and A mark the poles of the geotectonic axis PA.