x_over
x_over - Find and compute Cross-Over Errors
SYNOPSIS
x_over leg_1 [ leg_2 ] [ -A ] [ -C ] [ -L ] [ -V ] [
-Wtimegap ] [ -Gfact ] [ -Mfact ] [ -Tfact ] [ -Nnp_int ]
DESCRIPTION
x_over is used to inspect two cruises to see if they
intersect, and if so report the time, position, discrepan
cies in gravity/magnetics/bathymetry, heading for each
track segment, and the average values of the geophysical
observables at the cross-over point. The names of the legs
are passed on the command line. If they are identical or
only one name is passed, then x_over looks for internal
cross-overs. The optional parameters are:
-A Use Akima's spline to interpolate the geophysical
field at the cross-over point.'
-C Use a Natural Cubic spline function instead.
-L Use a linear interpolant [Default].
-W Do not compute cross-overs if the 2 nearest points
are more than timegap minutes apart.
-G Scale gravity by fact [Default is 0.1 since gmt-
files store gravity in g.u.]
-M Scale magnetic anomaly by fact [1.0].
-T Scale bathymetry by fact [1.0].
-N Specify how many points to use in the interpolation
[Default is 6].
-V Verbose, report the number of cross-overs for this
pair of legs.
The COEs found are printed out to standard output in ASCII for
mat. The first record contains the
leg names and their start year, whereas subsequent records
have the data for each COE encountered. The fields written
out are lat, lon, time along track #1, time along track
#2, x_gravity, x_magnetics, x_bathymetry, average gravity,
average magnetics, average bathymetry, heading along track
#1, and heading along track #2. Sign convention: If lega
and legb are passed on the command line, then the COE
value is Value (lega) - Value (legb). It is recommended
that the Akima's spline is used instead of the natural
cubic spline, since it is less sensitive to' outliers that
tend to introduce wild oscillations in the interpolation.
SEE ALSO
gmt(l), x_system(l)
REFERENCES
Wessel, P. XOVER: A Cross-over Error Detector for Track
Data, Computers & Geosciences, 15, 333-346.
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