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    Gravimetric geoid refinement using high resolution gravity and terrain data

    146672_24804_improv.pdf (261.3Kb)
    Access Status
    Open access
    Authors
    Featherstone, Will
    Alexander, K.
    Sideris, M.
    Date
    1996
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Featherstone, Will and Alexander, Ken and Sideris, Michael. 1996. Gravimetric geoid refinement using high resolution gravity and terrain data. Geomatics Research Australasia. 64: pp. 75-99.
    Source Title
    Geomatics Research Australasia
    ISSN
    13249983
    Faculty
    Department of Spatial Sciences
    Faculty of Science and Engineering
    WA School of Mines
    Remarks

    Geomantics Research Australasia has been succeeded by Journal of Spatial Science.

    URI
    http://hdl.handle.net/20.500.11937/17359
    Collection
    • Curtin Research Publications
    Abstract

    In regions where additional, spatially dense gravity and terrain information are available to augment existing data, a gravimetric determination of the geoid can be improved by incorporating these new data. In this study, 4,016 additional gravity observations, measured on a near-regular 2km by 3km grid in Western Australia have been used to compute a gravimetric geoid model using fast Fourier transform (FFT) techniques. A digital terrain model is also used during the geoid computations, which is derived from gravity station elevations and spot heights in the area. Using 21 spirit-levelled Australian Height Datum (AHD) heights in conjunction with Global Positioning System (GPS) ellipsoidal heights as control data, the standard deviation of the new gravimetric geoid is ±0.0824m. This represents a 31% improvement over the existing AUSGEOID93 gravimetric geoid and a 48% improvement over the OSU91A global geopotential model. Of these improvements, approximately 10% is due to the additional gravity data and approximately 1% is due to the terrain effects; the remainder is due to the dense gridding of the data prior to the FFT computations.

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