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Grand Challenges for EarthScope in Geodesy

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Title: Grand Challenges for EarthScope in Geodesy


1
Grand Challenges for EarthScope in Geodesy
  • Jim Davis
  • Harvard-Smithsonian Center for Astrophysics

2
Bennett et al. 2003
3
GPS Horizontal Velocity Errorsseven-year timespan
4
white noise error correlated error
120-d boxcar smoothing
5
Time-Correlated Site Motions
  • Our tectonic framework predicts (generally)
    time-linear site motions
  • Exceptions coseismic, postseismic, magmatic
    events
  • Nonlinear site motions (even if real) ? geodetic
    error
  • Power spectra of nonlinearities are used to
    derive error models ?

6
  • Deformation interpret-ed as periodic slow
    earthquakes in Cas-cadia subduction zone Miller
    et al., 2002?
  • More recently, defor-mation associated with
    tremor activity

7
  • Deformation associated with deep swarm of M lt 2.2
    earthquakes beneath Lake Tahoe
  • GPS measurements at BARGEN site SLID compared to
    cumula-tive moment ?
  • From Smith et al., submitted

8
  • Temporally nonlinear motions of BARGEN sites
    modeled with acceleration terms
  • See Davis and Wernicke poster

9
Great Salt Lake Loading
Elósegui et al. 2003.
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Grand Geodetic Questions for EarthScope
  • Under what conditions, and on what time and space
    resolution and scales, is crustal deformation
    continuous and secular?
  • Is the time-linearity default simply a
    convenient approximation for the Earths behavior
    in the era of gt1 mm/yr level (campaign)
    geodesy?
  • What can this nonsecular behavior tell us about
    forces in the Earths crust and interior and the
    response of the crust to those forces?

14
Challenges for Geodesy
  • Quantify (accurately) GPS error and its temporal
    and spatial behavior
  • Must be independent (as possible) of assumptions
    concerning Earths behavior
  • Will rely heavily on multiple techniques and data
    types
  • Must be applicable to EarthScopes spatial and
    temporal scales (inner and outer)
  • Develop analysis strategies that allow for
    non-secular behavior

15
Conclusions from Early Space Geodetic Work
  • Global plate motion is ongoing
  • Plate tectonic motion is continuous and linear
  • Exceptions are known episodic events
  • At right Figure from Larson et al. 1997
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