X2SYS_SOLVE(1gmt) | GMT | X2SYS_SOLVE(1gmt) |
x2sys_solve - Determine least-squares systematic correction from crossovers
x2sys_solve -Ccolumn -TTAG -Emode [ COE_list.d ] [ -V[level] ] [ -W[u] ] [ -bibinary ] [ -dinodata ] [ -x[[-]n] ]
Note: No space is allowed between the option flag and the associated arguments.
x2sys_solve will use the supplied crossover information to solve for systematic corrections that can then be applied per track to improve data quality. Several systematic corrections can be solved for using a least-squares approach. Note: Only one data column can be processed at the time.
c will fit f(p) = a (a constant offset); records must contain track ID1, ID2, COE.
d will fit f(p) = a + b * d (linear drift; d is distance; records must contain track ID1, ID2, d1, d2, COE.
g will fit f(p) = a + b sin(y)^2 (1980-1930 gravity correction); records must contain track ID1, ID2, latitude y, COE.
h will fit f(p) = a + b cos(H) + c cos(2H) + d sin(H) + e sin(2H) (magnetic heading correction); records must contain track ID1, ID2, heading H, COE.
s will fit f(p) = a * z (a unit scale correction); records must contain track ID1, ID2, z1, z2.
t will fit f(p) = a + b * (t - t0) (linear drift; t0 is the start time of the track); records must contain track ID1, ID2, t1-t0, t2-t0, COE.
Most of the model corrections in -E involve a constant offset. Because crossovers are differences between values, any absolute level will cancel out and hence the constant offsets we obtain are relative to an undetermined absolute level. To obtain a solvable solution we add the constraint that the sum of all constant offsets equal zero. If the tracks form clusters in which no tracks from one cluster cross any track from another cluster then these are two independent data sets and require they own constraint equation for their offsets. We determine the number of clusters and automatically add the required constraint equations. If you need a particular reference track to have a particular offset (e.g., 0) then you can subtract the offset you found from every track correction and add in the desired offset.
To fit a simple bias offset to faa for all tracks under the MGD77 tag, try
gmt x2sys_list COE_data.txt -V -TMGD77 -Cfaa -Fnc > faa_coe.txt gmt x2sys_solve faa_coe.txt -V -TMGD77 -Cfaa -Ec > coe_table.txt
To fit a faa linear drift with time instead, try
gmt x2sys_list COE_data.txt -V -TMGD77 -Cfaa -FnTc > faa_coe.txt gmt x2sys_solve faa_coe.txt -V -TMGD77 -Cfaa -Et > coe_table.txt
To estimate heading corrections based on magnetic crossovers associated with the tag MGD77 from the file COE_data.txt, try
gmt x2sys_list COE_data.txt -V -TMGD77 -Cmag -Fnhc > mag_coe.txt gmt x2sys_solve mag_coe.txt -V -TMGD77 -Cmag -Eh > coe_table.txt
To estimate unit scale corrections based on bathymetry crossovers, try
gmt x2sys_list COE_data.txt -V -TMGD77 -Cdepth -Fnz > depth_coe.txt gmt x2sys_solve depth_coe.txt -V -TMGD77 -Cdepth -Es > coe_table.txt
x2sys_binlist, x2sys_cross, x2sys_datalist, x2sys_get, x2sys_init, x2sys_list, x2sys_put, x2sys_report
2019, P. Wessel, W. H. F. Smith, R. Scharroo, J. Luis, and F. Wobbe
May 21, 2019 | 5.4.5 |