GLOBK%20Velocity%20Solutions - PowerPoint PPT Presentation

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GLOBK%20Velocity%20Solutions

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Generating realistic velocity sigmas (eariler lecture) ... sh_gen_stats to get process noise on the sites and get lists fo stabile sites. ... – PowerPoint PPT presentation

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Title: GLOBK%20Velocity%20Solutions


1
GLOBK Velocity Solutions
  • Thomas Herring

2
Overview
  • Basic velocity solution
  • Generating realistic velocity sigmas (eariler
    lecture)
  • Accounting for earthquakes and site offsets
  • Pre-stacking and speeding up results

3
Basic velocity solution
  • Basic process is
  • Make a file with list of binary h-files (usually
    .glx files). These hfiles span multiple years
    normally
  • glist can be used to see list of stations and
    durations and check for large differences in
    coordinates.
  • globk command file add
  • apr_neu all 10 10 10 1 1 1
  • Assigns 1 m/yr uncertainty to velocities at all
    sites
  • glorg command file add
  • rate_org xtran ytran ztran ltxrotgt ltyrotgt ltzrotgt
    ltscalegt
  • Entries depend on if rotations and scale are
    estimated in globk

4
Basic solution Orbits
  • Considerations in globk
  • If Choice of Experiment RELAX in sestbl. then
    orbits needed to accounted for.
  • Merge with global orbit files (available from MIT
    as combined binary h-files)
  • Constrain or fix the orbits. Post-2000 IGS
    orbits can generally be fixed,
  • There are advatages to generated updated h-files
    with orbits contsrained or fixed. (Speeds up
    velocity solution because apr_svs command not
    needed in velocity solution).
  • If Choice of Experiment BASELINE then orbits
    are fixed so do not need to be treated specially.
  • With older data (pre-2000) still useful to
    estimate orbits. Also depends on next size
    (lt1000km).

5
Basic solution EOP
  • When RELAX mode, EOP parameters (apr_wob and
    apr_ut1) are estimated when BASELINE mode used,
    they are not estimated in gamit and therefore
    orientation of system is fixed.
  • If apr_wob/apr_ut1 used, then mar_wob and mar_ut1
    should also be used to allow these to vary with
    time.
  • For long baselines and BASELINE mode, these
    should be included in command file.
  • For short baselines (lt1000km) and RELAX mode,
    they can be not included (not further
    constraint), or constrained (even F is OK).
  • When tightly constrained (lt0.2 mas), xrot yrot
    zrot should be included in pos/rate_org commands

6
Basic Solution Scale
  • Treatment of scale is unclear as to best approach
  • For long baseline and long time series, apr_scale
    and mar_scale probably should be used until
    re-processed IGS products are available.
  • Shorter baseline, probably dont need scale
    estimated.
  • Suggestion is to try both ways and see impact on
    results (good use of OPTION string in globk and
    glorg command files).

7
Accounting for earthquakes and site offsets
  • Earthquakes and offsets are accounted for with
    the eq_file.
  • Generally, after and earthquake there is
    post-seismic motion which can be accounted for
    with the eq_post process noise or eq_log log
    estimates.
  • Parameters for some earthquakes are given in
    distributed tables directory. Ideally for other
    earthquakes, model for coseismic motion can be
    used to determine parameters, Postseismic is
    often assumed to 10-20 of coseismic.
  • The glorg commends equate and eq_dist can be used
    to make velocities the same before and after
    offsets. Apriori velocity be the same FIXA
    org_opt can bs used but should be checked.

8
Offsets
  • The RNRP org_opt can be used to get an estimate
    of the offset magnitude to see if it is
    significant.
  • The script sh_exeqs can be used to extract equate
    lines from glorg output. These can be used then
    in glorg to apply equates.

9
Pre-stacking and speeding up results
  • With large numbers of days of data and stations,
    velocity solutions can take a long time. Some
    methods of speeding up runs
  • The globk command use_num can specify the minimum
    number of times a site is used. Also glist
    output can be used for this (with grep and awk)
  • The command decimate to process every nth file.
    With process noise, decimation make little
    difference to results. (decimate 7 or even 30
    works well with continuous data).

10
Pre-stacking
  • Pre-stacking hfiles also works well
  • Several approaches here
  • Combination of local and global hfiles to get
    orbits
  • Orbits loose in combination and then not used
    afterwards (I.e., no further constraints)
  • Combined hfiles or individual hfiles can be
    combined in time to form n-day averages (7 to 30
    days work fine).
  • With process noise used 7-30 day combination
    should estimate only position and not velocity.
    MIDP org_opt will refer result to center of data
    span.
  • Same process noise model should be used when
    making 7-30 day combination and when combining
    the combined h-files. (Statistically, the
    results are same as direct solution)
  • Care needed in duration of combinations during
    times of large post-seismic deformation (use
    shorter combinations)
  • With time-stacks, the chi2 increments will be
    greater than 1 because random walk is too step a
    spectrum.

11
Extracting and displaying results
  • There are shell scripts to extract results (e.g.,
    sh_exglk) and shell scripts to plot velocity
    field (e.g., sh_plotvel)
  • velview and tsview can be used to display
    velocities and time series.
  • tsview outputs rename files that can be used in
    globk. It can also read an eq_file from globk to
    apply breaks and earthquakes.

12
Iteration of results
  • Common approach is to
  • Run velocity solution and extract coordinates for
    new apriori coordinate file.
  • Use this new apr_file and good stations to
    generate time series with glred.
  • Use sh_gen_stats to get process noise on the
    sites and get lists fo stabile sites. Command
    sig_neu can used to account for occasional error
    such as campaign with bad height,
  • Use these estimates to re-estimate velocity and
    iterate the system
  • Time series can be used to detect outliers (use
    rename to ltnamegt_XCL or ltnamegt_XPS in eq_file)
    and breaks (can rename in eq_file to ltnamegt_?PS
    where ? Is letter or number)

13
Summary
  • Basic velocity solution Useful when small number
    of days and stations.
  • Accounting for earthquakes and site offsets
  • Can be complex with large data sets
  • Use source command to allow reading in of
    standard values. Runstring option can be used to
    have same command file for velocity and
    repeatability runs
  • Pre-stacking and speeding up results Useful with
    large continuous data solutions. Multiple
    techniques can be used.
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