Provided by: gmt-common_5.4.3+dfsg-1_all 
NAME
blockmode - Block average (x, y, z) data tables by mode estimation
SYNOPSIS
blockmode [ table ]
-Iincrement
-Rregion [ -C ] [ -D[width][+c][+a|+l|+h ] [ -Er|s[-] ] [ -Q ] [ -V[level] ] [ -W[i|o][+s] ] [
-bbinary ] [ -dnodata ] [ -eregexp ] [ -fflags ] [ -hheaders ] [ -iflags ] [ -oflags ] [ -r ] [ -:[i|o] ]
Note: No space is allowed between the option flag and the associated arguments.
DESCRIPTION
blockmode reads arbitrarily located (x,y,z) triples [or optionally weighted quadruples (x,y,z,w)] from
standard input [or table] and writes to standard output mode estimates of position and value for every
non-empty block in a grid region defined by the -R and -I arguments. Either blockmean, blockmedian, or
blockmode should be used as a pre-processor before running surface to avoid aliasing short wavelengths.
These routines are also generally useful for decimating or averaging (x,y,z) data. You can modify the
precision of the output format by editing the FORMAT_FLOAT_OUT parameter in your gmt.conf file, or you
may choose binary input and/or output to avoid loss of precision.
REQUIRED ARGUMENTS
-Ixinc[unit][+e|n][/yinc[unit][+e|n]]
x_inc [and optionally y_inc] is the grid spacing. Optionally, append a suffix modifier.
Geographical (degrees) coordinates: Append m to indicate arc minutes or s to indicate arc seconds.
If one of the units e, f, k, M, n or u is appended instead, the increment is assumed to be given
in meter, foot, km, Mile, nautical mile or US survey foot, respectively, and will be converted to
the equivalent degrees longitude at the middle latitude of the region (the conversion depends on
PROJ_ELLIPSOID). If y_inc is given but set to 0 it will be reset equal to x_inc; otherwise it will
be converted to degrees latitude. All coordinates: If +e is appended then the corresponding max x
(east) or y (north) may be slightly adjusted to fit exactly the given increment [by default the
increment may be adjusted slightly to fit the given domain]. Finally, instead of giving an
increment you may specify the number of nodes desired by appending +n to the supplied integer
argument; the increment is then recalculated from the number of nodes and the domain. The
resulting increment value depends on whether you have selected a gridline-registered or
pixel-registered grid; see App-file-formats for details. Note: if -Rgrdfile is used then the grid
spacing has already been initialized; use -I to override the values.
-Rxmin/xmax/ymin/ymax[+r][+uunit] (more …)
Specify the region of interest.
OPTIONAL ARGUMENTS
table 3 [or 4, see -W] column ASCII data table file(s) [or binary, see -bi] holding (x,y,z[,w]) data
values. [w] is an optional weight for the data. If no file is specified, blockmode will read from
standard input.
-C Use the center of the block as the output location [Default uses the modal xy location (but see
-Q)]. -C overrides -Q.
-D[width][+c][+a|+l|+h ]
Perform unweighted mode calculation via histogram binning, using the specified histogram width.
Append +c to center bins so that their mid point is a multiple of width [uncentered]. If multiple
modes are found for a block we return the average mode [+a]. Append +l or +h to return the low of
high mode instead, respectively. If width is not given it will default to 1 provided your data
set only contains integers. Also, for integer data and integer bin width we enforce bin centering
(+c) and select the lowest mode (+l) if there are multiples. [Default mode is normally the Least
Median of Squares (LMS) statistic].
-E Provide Extended report which includes s (the L1 scale of the mode), l, the lowest value, and h,
the high value for each block. Output order becomes x,y,z,s,l,h[,w]. [Default outputs x,y,z[,w].
See -W for w output.
-Er|s[-]
Provide source id s or record number r output, i.e., append the source id or record number
associated with the modal value. If tied then report the record number of the higher of the two
values; append - to instead report the record number of the lower value. Note that both -E and
-Er[-] may be specified. For -Es we expect input records of the form x,y,z[,w],sid, where sid is
an unsigned integer source id.
-Q (Quicker) Finds mode z and mean (x,y) [Default finds mode x, mode y, mode z].
-V[level] (more …)
Select verbosity level [c].
-W[i|o][+s]
Weighted modifier[s]. Unweighted input and output have 3 columns x,y,z; Weighted i/o has 4 columns
x,y,z,w. Weights can be used in input to construct weighted modal values for each block. Weight
sums can be reported in output for later combining several runs, etc. Use -W for weighted i/o, -Wi
for weighted input only, and -Wo for weighted output only. [Default uses unweighted i/o]. If your
weights are actually uncertainties (one sigma) then append +s and we compute weight = 1/sigma.
-bi[ncols][t] (more …)
Select native binary input. [Default is 3 (or 4 if -Wi is set)].
-bo[ncols][type] (more …)
Select native binary output. [Default is 3 (or 4 if -Wo is set)]. -E adds 3 additional columns.
-d[i|o]nodata (more …)
Replace input columns that equal nodata with NaN and do the reverse on output.
-e[~]”pattern” | -e[~]/regexp/[i] (more …)
Only accept data records that match the given pattern.
-f[i|o]colinfo (more …)
Specify data types of input and/or output columns.
-h[i|o][n][+c][+d][+rremark][+rtitle] (more …)
Skip or produce header record(s).
-icols[+l][+sscale][+ooffset][,…] (more …)
Select input columns and transformations (0 is first column).
-ocols[,…] (more …)
Select output columns (0 is first column).
-r (more …)
Set pixel node registration [gridline]. Each block is the locus of points nearest the grid value
location. Consider an example with -R10/15/10/15 and -I1: With the -r option, 10 <= (x,y) < 11 is
one of 25 blocks; without it 9.5 <= (x,y) < 10.5 is one of 36 blocks.
-:[i|o] (more …)
Swap 1st and 2nd column on input and/or output.
-^ or just -
Print a short message about the syntax of the command, then exits (NOTE: on Windows just use -).
-+ or just +
Print an extensive usage (help) message, including the explanation of any module-specific option
(but not the GMT common options), then exits.
-? or no arguments
Print a complete usage (help) message, including the explanation of all options, then exits.
ASCII FORMAT PRECISION
The ASCII output formats of numerical data are controlled by parameters in your gmt.conf file. Longitude
and latitude are formatted according to FORMAT_GEO_OUT, absolute time is under the control of
FORMAT_DATE_OUT and FORMAT_CLOCK_OUT, whereas general floating point values are formatted according to
FORMAT_FLOAT_OUT. Be aware that the format in effect can lead to loss of precision in ASCII output, which
can lead to various problems downstream. If you find the output is not written with enough precision,
consider switching to binary output (-bo if available) or specify more decimals using the
FORMAT_FLOAT_OUT setting.
EXAMPLES
To find 5 by 5 minute block mode estimates from the double precision binary data in hawaii_b.xyg and
output an ASCII table, run:
gmt blockmode hawaii_b.xyg -R198/208/18/25 -I5m -bi3d > hawaii_5x5.xyg
To determine the most frequently occurring values per 5x5 block using histogram binning, with data
representing integer counts, try
gmt blockmode data.txt -R0/100/0/100 -I5 -r -C -D
SEE ALSO
blockmean, blockmedian, gmt, gmt.conf, greenspline, nearneighbor, sphtriangulate, surface, triangulate
COPYRIGHT
2018, P. Wessel, W. H. F. Smith, R. Scharroo, J. Luis, and F. Wobbe