backtracker
backtracker - Forward and Backward flowlines and hotspot
tracks
SYNOPSIS
backtracker [infile(s)] -Estage_file [ -A[young/old] ] [
-C ] [ -Df|b ] [ -H[nrec] ] [ -Lf|tstep ] [ -Nupper_age ]
[ -Sfilestem ] [ -Tzero_age ] [ -V ] [ -: ] [ -bi[s][n] ]
[ -bo[s] ]
DESCRIPTION
backtracker reads (longitude, latitude, age) positions
from infiles [or standard input] and computes projected
(x,y,t) coordinates using the specified stage pole (Euler)
rotations. You can either calculate just final positions
[Default] or create a sampled track between initial and
final position. The former mode allows additional data
fields after the first 3 columns which must have (longi
tude,latitude,age). See option -: on how to read (lati
tude,longitude,age) files.
No space between the option flag and the associ
ated arguments. Use upper case for the option flags and
lower case for modifiers.
infile(s)
Data file(s) to be projected. If not given, stan
dard input is read.
-E Give file with stage poles and opening angles. This
file must contain one record for each stage; each
record must be of the following format:
lon lat tstart tstop ccw-angle
where time is in Ma and the rest is in degrees.
Oldest stage must be listed first. tstart is the
time when the stage begins (oldest age). Blank
lines and records whose first column contains #
will be ignored.
OPTIONS
-A Used in conjunction with -Lb|f to limit the track
output to those sections whose predicted ages fit
between the young and old limits. If -LB|F is used
instead then the limits apply to the stage ids. If
no limits are supplied then individual limits for
each seamount are expected in the input file's
columns 4 and 5.'
-C Expect Total Reconstruction Poles (Finite Poles)
rather than Backward Stage Poles [Default] File
format is similar to the stage pole format except
the youngest rotation must be listed first and that
time, while -Db will go backward in time [Default].
-H Input file(s) has Header record(s). Number of
header records can be changed by editing your .gmt
defaults file. If used, GMT default is 1 header
record.
-L Specify a sampled path between initial and final
position: -Lf will draw flowlines, while -Lb will
draw backtrack (hotspot track) paths. Append sam
pling interval in km. When -LF or -LB is used, the
third output column will contain the stage id (1 is
youngest) [Default is along-track ages].
-N Set the maximum age to extend the oldest stage back
in time [Default is no extension].
-S When -L is set, the tracks are normally written to
stdout as a multisegment file. Specify a filestem
to have each track written to filestem.#, where #
is the track number. The track number is also
copied to the 4th output column.
-T Set the current time [Default is 0 Ma].
-V Selects verbose mode, which will send progress
reports to stderr [Default runs "silently"].
-: Toggles between (longitude,latitude) and (lati
tude,longitude) input/output. [Default is (longi
tude,latitude)]. Applies to geographic coordinates
only.
-bi Selects binary input. Append s for single precision
[Default is double]. Append n for the number of
columns in the binary file(s). [Default is 3 input
columns].
-bo Selects binary output. Append s for single preci
sion [Default is double].
EXAMPLES
To backtrack the (x,y,t) points in the file seamounts.d to
their origin (presumably the hotspot), using the DC85.d
Euler poles, run
backtracker seamounts.d -Db -EDC85.d > newpos.d
To project flowlines forward from the (x,y,t) points
stored in several 3-column, binary, double precision
files, run
SEE ALSO
gmt(l), project(l), mapproject(l), hotspotter(l) origina
tor(l)
REFERENCES
Wessel, P., 1999, "Hotspotting" tools released, EOS Trans.
AGU, 80 (29), p. 319.
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