The document discusses Geoscience Australia's work with gravity data, including airborne and satellite gravity. It aims to improve national gravity databases by expanding coverage and enhancing modeling capabilities. Key efforts include supporting airborne gravity surveys, developing a test site to evaluate new technologies, maintaining fundamental gravity networks, and improving 3D modeling through national and international collaborations.
Australia has a land area of 7,617,930 km2 (http://en.wikipedia.org/wiki/Australia), but we have direct interest in a further 8,148,250 km2 that falls within our Exclusive Economic Zone (http://en.wikipedia.org/wiki/Exclusive_Economic_Zone#Australia).
AGG onshore coverage @$100/line km and line spacing of 1 km = A$750 M
AG coastal and offshore coverage @$50/line km and line spacing of 2 km = A$250 M
Total coverage costs = A$1 B
GRACE - Gravity Recovery and Climate Experiment
US and German space agencies (NASA and DLG)
Launched March 2002.
Orbiting at an approximate altitude of 485 km.
Two satellites separated by approximately 220 km (“Tom” and “Jerry”).
Separation monitored by microwave ranging to an accuracy of approximately 10 microns.
Position of the satellites monitored using GPS navigation.
Accelerometers onboard each satellite provide total acceleration, simply as a cross-check on the gravity determinations.
Providing both mean global gravity fields and monthly estimates of the temporal variations in the force of gravity.
Approximately 400 km horizontal spatial resolution.
Applications
Global mean gravity field maps
Geoid determination
Temporal variations in the Earth’s mass distribution
(e.g., water storage changes – surface, groundwater, ice sheets and glaciers; sea level changes; tectonic movements)
10 nms-2 change in gravity is approximately equivalent to 24 mm of water.
Opportunities for GA
Custodian of national gravity information
Long wavelength mean gravity fields for the Australian region
Temporal changes in gravity for accurate corrections to gravity measurements
Support for users of temporal gravity variations
Support for geodetic applications (e.g., coastal regions, Antarctica)
http://www.csr.utexas.edu/grace/
http://en.wikipedia.org/wiki/Gravity_Recovery_and_Climate_Experiment
GOCE - Gravity Field and Steady-State Ocean Circulation Explorer
European Space Agency (ESA)
Launched March 2009.
Orbiting at an approximate altitude of 260 km.
Gravity gradients measured by an EGG (Electrostatic Gravity Gradiometer)
Repeat orbit every 61 days.
Position of the satellite monitored using GPS navigation.
Providing both mean global gravity fields and monthly estimates of the temporal variations in the force of gravity.
Approximately 100 km horizontal spatial resolution.
Anticipated accuracy of ~ 1 mGal with 100 km resolution
c/f GRACE – lower altitude and gradient measurement = superior spatial resolution
First preliminary global models released June 2010 – currently being analysed
http://earth.esa.int/GOCE/
http://en.wikipedia.org/wiki/GOCE
The GGM 03S solution is a Grace only solution, which is complete to degree and order 180. The GGM 03C solution is obtained by combining the information arrays from the GGM 03S solution with surface gravity data to obtain a solution complete to degree and order 360. The higher resolution detail in the 03C solution represents the contribution of the surface gravity data ti the very accurate long and mid wave length GRACE data.
THE COMBINATION GRAVITY FIELD MODEL GGMO3C
Reference: B. Tapley, J. Ries, S. Bettadpur, D. Chambers, M. Cheng, F. Condi, S. Poole, 2007, The GGM03 Mean Earth Gravity Model from GRACE: Eos Trans. AGU 88(52), Fall Meet. Suppl., Abstract G42A-03, 2007.
GGMO3C is a combination of GRACE gravity information from GGMO3S) with land and ocean gravity information, complete to degree and order 360. GGMO3S was determined from 47 months of GRACE K-band intersatellite range-rate data, GPS tracking and GRACE accelerometer data spanning the period from January 2003 through December 2006 (January 2004 excluded). The terrestrial gravity information was a combination of the NINA surface gravity anomalies, the CSR mean sea surface (MSS95), and the Arctic Gravity Project (ArcGP) gravity anomalies. GGM031 was used to fill where no terrestrial gravity information was available. The GRACE atmosphere-ocean de-aliasing product (A0D1B) was used, but the mean of the A0D1B for the 47 months has been restored. Please Note: the reference epoch of this mean gravity field model is 1 January 2005. Terms for which rates were modeled have been mapped to this epoch; these include C20, C30, C40, C21 and S21. For additional details on the background modeling, see the CSR RL04 processing standards document available at ...
ftp://podaac.jpl.nasa.govipubigraceidoc/L2-CSR0004_ProcStd_v3.1.pdf
Product type: gravity field
Model name: GGMO3C
Earth gravity constant: 0.3986004415E+15
Tracey R, Bacchin M & Wynne P. 2008. AAGD07: A new absolute gravity datum for Australian gravity and new standards for the Australian National Gravity Database. Extended Abstracts, 19th International Geophysical Conference and Exhibition. Australian Society of Exploration Geophysicists.
Tracey R & Nakamura A. 2010. Complete Bouguer Anomalies for the Australian National Gravity Database: Extended Abstracts, 21st International Geophysical Conference and Exhibition. Australian Society of Exploration Geophysicists.
First absolute gravity measurements in the Australian Antarctic Territory
Geoscience Australia has recently conducted absolute gravity observations at Davis and Mawson stations in the Australian Antarctic Territory. These observations are the first such measurements undertaken at any of the Australian Antarctic stations to establish accurate gravity reference points for future gravity surveys. They will also enable gravity surveys that have already been conducted in the Australian Antarctic Territory to be tied to the same datum, thus allowing previous and future gravity surveys to be accurately merged and combined.
Figure 1. Ties between existing gravity base stations and the new absolute gravity base stations were conducted using a relative gravity meter.
Gravity reference points (or gravity base stations) have been established at the Australian Antarctic stations in the past but these were done with relative gravity meters. These instruments measure the difference in gravity from one point to another and were used to measure the difference between a reference point in Australia and the reference points that had been established in Antarctica. Unfortunately the length of time involved in travelling to Antarctica combined with 'instrumental drift' was not conducive to accurate readings so the accuracy of these older reference points was compromised.
Figure 2. Map showing the location of Davis and Mawson in relation to Australia and the track of the RSV Aurora Australis during Voyage 3, 2009-10.
The absolute gravity meter determines the actual acceleration of gravity by measuring the trajectory of a free-falling object in a vacuum. The surviving gravity base stations at Davis and Mawson were tied to the new absolute base stations using a relative gravity meter (figure 1). Gravity surveys that used these old reference points can now be adjusted to the new absolute datum.
Transport to and from the Antarctic stations was onboard the Australian Antarctic Division's re-supply vessel RSV Aurora Australis, which departed Hobart on 25 January 2010 and returned on 28 February 2010. The ship's track for this voyage and the location of Davis and Mawson can be seen in figure 2.
For more information Ray Tracey on +61 2 6249 9111 (email ray.tracey@ga.gov.au)
20081015
What's so fundamental about a gravity network?
Presenter - Ray Tracey, OEMD
Abstract
The Australian Fundamental Gravity Network (AFGN) provides the datum for gravity surveys conducted in Australia and the surrounding oceans. It consists of more than 900 gravity stations at over 250 locations. The network was initially established in the early 1950s with stations added at various times up to the present. All of these stations were established using relative gravimeters to measure gravity differences between stations.
Relative gravimeter ties to overseas gravity stations were used to establish the gravity datum prior to 1979 when five absolute gravity sites were established in Australia with a Soviet absolute gravimeter. These sites were tied to the network and used to constrain the Isogal84 datum, which was in use from 1984 until 2008.
Between 2003 and 2006 Geoscience Australia conducted absolute gravity measurements with a portable absolute gravimeter at 60 AFGN stations. These measurements showed that there was a consistent difference between the Isogal84 datum and the absolute measurements. These measurements have been used to establish a new datum, the Australian Absolute Gravity Datum 2007 (AAGD07), and to adjust the Australian National Gravity Database (ANGD) to this new datum.
Concurrent with implementing AAGD07, the standards used for reducing gravity data in the ANGD have been reviewed and updated. These changes include using the closed form of the 1980 International Gravity Formula, global horizontal and vertical datums, and a spherical cap Bouguer correction that accounts for the Earth's curvature. These new standards provide more accurate anomalies, particularly in longer wavelengths thus benefiting regional studies.
This talk presents an abridged history of the AFGN explaining the new datum and standards and showing why the AFGN is fundamental to Australian gravity.
Biography
Ray Tracey is a geophysicist in the Continental Geophysics Project in OEMD where he is responsible for the maintenance of the Australian Fundamental Gravity Network. He started work with BMR/AGSO/GA in 1975 as a Trainee Technical Officer and gained experience in a number of different areas of the Bureau during the traineeship. After completing his traineeship he conducted numerous gravity surveys in many out of the way parts of the country before being foolish enough to accept the pieces of silver on offer to join the crew on BMR's marine research vessel, Rig Seismic. After experiencing life on the high seas for a number of years, he jumped ship and returned to solid land and the more stable lifestyle of gravity surveying. Along the way, Ray has acquired a computing and remote sensing degree from the University of Canberra and a Master of Geoscience from Macquarie University
Philosophers and seafarers in ancient Greek and Egyptian civilizations were aware of it from the 6th century BC onwards.
The circumnavigation of the Earth in the early 16th century by members of Ferdinand Magellan’s voyage made it really difficult to ignore.
Pilots and astronauts could see directly that it is true from high altitude and space in the 20th century.
Here in the 21st century, few of us doubt that it is true.
What am I talking about? We carry out our modelling using rectangular “flat Earth” coordinate systems. But the Earth is more like a sphere than a slab.
So rather than simply continue to perform all of our gravity and magnetic modelling in Cartesian “flat Earth” coordinate reference frameworks, we are collaborating with a number of groups spread right across the globe to implement modelling options that use a spherical reference framework.
40 degrees E to 180 degrees E
0 degrees to 90 degrees S
Australia's Maritime Jurisdiction spans nearly ¼ of the globe.
CUG-CSM-GA International project for spherical mesh geometry gravity and magnetic modeling
CUG – China University of Geosciences
CSM – Colorado School of Mines
GA – Geoscience Australia
Our Memorandum-Of-Understanding (MOU) signed on 11-October-2011 ...
"Our respective organizations acknowledge a commitment to pursue an agreement for international collaboration on the modeling and application of gravity and magnetic data in a spherical mesh geometry. We shall work together in good spirit and faith to finalize an agreement, and if this is successful, to then carry out the project. We commit to work to the benefit of the collective group, recognizing that this will produce the greatest overall benefit to the individual interests of each of the constituent parties over the full course of the collaborative project.“
Richard Lane (Geoscience Australia)
Yaoguo Li (Colorado School of Mines)
Chao Chen and Qing Liang (China University of Geosciences)
(From a presentation prepared by Qing Liang titled “3-D inversion of gravity data in spherical coordinate: Modeling the density structure of planetary lithosphere”)
Chen, C., Chen, B., and Ping, J. S., Liang, Q., Huang, Q., And Zhao, W. J., 2009, The interpretation of gravity anomaly on lunar Apennines: Science in China Series G: Physics, Mechanics & Astronomy, 52(12), 1824-1832, doi: 10.1007/s11433-009-0281-0.
Du., J. S., Chen, C., Liang, Q., and Zhou, C., 2011, Lateral density variations on the surface and in the crust of the Moon: The 42nd Lunar and Planetary Science Conference, The Woodlands, Texas, USA, March 7–11, Abstract #1744.
Liang, Q., 2010, Gravity anomaly features and 3D density imaging of the Moon: PhD dissertation, China University of Geosciences (Wuhan), Wuhan, China.
Liang, Q., Chen, C., and Du, J., Chen, B., 2009, Calculation of lunar Bouguer gravity anomaly using Chang'E-1 topography data: Interpretation for mascons: Poster presented at the AGU Fall Meeting, San Francisco, California, USA.
Liang, Q., Chen, C., Huang, Q., Chen, B., and Ping, J. S., 2009, Bouguer gravity anomaly of the Moon from CE-1 topography data: Implications for the impact basin evolution: Science in China Series G: Physics, Mechanics & Astronomy, 52(12), 1867-1875, doi: 10.1007/s11433-009-0278-8.
Liang, Q., Chen, C., and Li, Y., 2010, 3D inversion of lunar gravity data and preliminary results: Poster presented at the AGU Fall Meeting, San Francisco, California, USA.
Liang, Q., Chen, C., and Li, Y., 2011, 3-D inversion of the gravity data on the moon: The 42nd Lunar and Planetary Science Conference, The Woodlands, Texas, USA, March 7–11, Abstract #1729.
(From a presentation prepared by Qing Liang titled “3-D inversion of gravity data in spherical coordinate: Modeling the density structure of planetary lithosphere”)
Chen, C., Chen, B., and Ping, J. S., Liang, Q., Huang, Q., And Zhao, W. J., 2009, The interpretation of gravity anomaly on lunar Apennines: Science in China Series G: Physics, Mechanics & Astronomy, 52(12), 1824-1832, doi: 10.1007/s11433-009-0281-0.
Du., J. S., Chen, C., Liang, Q., and Zhou, C., 2011, Lateral density variations on the surface and in the crust of the Moon: The 42nd Lunar and Planetary Science Conference, The Woodlands, Texas, USA, March 7–11, Abstract #1744.
Liang, Q., 2010, Gravity anomaly features and 3D density imaging of the Moon: PhD dissertation, China University of Geosciences (Wuhan), Wuhan, China.
Liang, Q., Chen, C., and Du, J., Chen, B., 2009, Calculation of lunar Bouguer gravity anomaly using Chang'E-1 topography data: Interpretation for mascons: Poster presented at the AGU Fall Meeting, San Francisco, California, USA.
Liang, Q., Chen, C., Huang, Q., Chen, B., and Ping, J. S., 2009, Bouguer gravity anomaly of the Moon from CE-1 topography data: Implications for the impact basin evolution: Science in China Series G: Physics, Mechanics & Astronomy, 52(12), 1867-1875, doi: 10.1007/s11433-009-0278-8.
Liang, Q., Chen, C., and Li, Y., 2010, 3D inversion of lunar gravity data and preliminary results: Poster presented at the AGU Fall Meeting, San Francisco, California, USA.
Liang, Q., Chen, C., and Li, Y., 2011, 3-D inversion of the gravity data on the moon: The 42nd Lunar and Planetary Science Conference, The Woodlands, Texas, USA, March 7–11, Abstract #1729.
(From a presentation prepared by Qing Liang titled “3-D inversion of gravity data in spherical coordinate: Modeling the density structure of planetary lithosphere”)
Chen, C., Chen, B., and Ping, J. S., Liang, Q., Huang, Q., And Zhao, W. J., 2009, The interpretation of gravity anomaly on lunar Apennines: Science in China Series G: Physics, Mechanics & Astronomy, 52(12), 1824-1832, doi: 10.1007/s11433-009-0281-0.
Du., J. S., Chen, C., Liang, Q., and Zhou, C., 2011, Lateral density variations on the surface and in the crust of the Moon: The 42nd Lunar and Planetary Science Conference, The Woodlands, Texas, USA, March 7–11, Abstract #1744.
Liang, Q., 2010, Gravity anomaly features and 3D density imaging of the Moon: PhD dissertation, China University of Geosciences (Wuhan), Wuhan, China.
Liang, Q., Chen, C., and Du, J., Chen, B., 2009, Calculation of lunar Bouguer gravity anomaly using Chang'E-1 topography data: Interpretation for mascons: Poster presented at the AGU Fall Meeting, San Francisco, California, USA.
Liang, Q., Chen, C., Huang, Q., Chen, B., and Ping, J. S., 2009, Bouguer gravity anomaly of the Moon from CE-1 topography data: Implications for the impact basin evolution: Science in China Series G: Physics, Mechanics & Astronomy, 52(12), 1867-1875, doi: 10.1007/s11433-009-0278-8.
Liang, Q., Chen, C., and Li, Y., 2010, 3D inversion of lunar gravity data and preliminary results: Poster presented at the AGU Fall Meeting, San Francisco, California, USA.
Liang, Q., Chen, C., and Li, Y., 2011, 3-D inversion of the gravity data on the moon: The 42nd Lunar and Planetary Science Conference, The Woodlands, Texas, USA, March 7–11, Abstract #1729.