1FILTER1D(1)                  Generic Mapping Tools                 FILTER1D(1)
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NAME

6       filter1d - Time domain filtering of 1-D time series
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SYNOPSIS

9       filter1d  [  infile  ]  -F<type><width>[mode]  [ -Dincrement ] [ -E ] [
10       -H[i][nrec] ] [ -Iignore_val ] [ -Llack_width ] [  -Nn_cols/t_col  ]  [
11       -Qq_factor  ]  [  -Ssymmetry_factor  ]  [  -Tstart/stop/int  ] [ -V ] [
12       -b[i|o][s|S|d|D[ncol]|c[var1/...]] ] [ -f[i|o]colinfo ]
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DESCRIPTION

15       filter1d is a general time  domain  filter  for  multiple  column  time
16       series  data.   The  user  specifies the number of columns of input and
17       which column is the time.  (See -N option below).  The  fastest  opera‐
18       tion  occurs  when the input time series are equally spaced and have no
19       gaps or outliers and the special options are not needed.  filter1d  has
20       options -L, -Q, and -S for unevenly sampled data with gaps.
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22       infile Multi-column  ASCII (or binary, see -b) file holding data values
23              to be filtered.
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25       -F     Sets the filter type.  Choose among convolution and non-convolu‐
26              tion  filters.  Append the filter code followed by the full fil‐
27              ter width in same units as time  column.  Available  convolution
28              filters are:
29              (b) Boxcar: All weights are equal.
30              (c) Cosine Arch: Weights follow a cosine arch curve.
31              (g) Gaussian: Weights are given by the Gaussian function.
32              (f) Custom: Instead of width give name of a one-column file with
33              your own weight coefficients.
34              Non-convolution filters are:
35              (m) Median: Returns median value.
36              (p) Maximum likelihood probability (a  mode  estimator):  Return
37              modal  value.   If  more  than one mode is found we return their
38              average value.  Append - or + to the filter width if you  rather
39              want to return the smallest or largest of the modal values.
40              (l) Lower: Return the minimum of all values.
41              (L) Lower: Return minimum of all positive values only.
42              (u) Upper: Return maximum of all values.
43              (U) Upper: Return maximum or all negative values only.
44              Upper  case  type  B,  C, G, M, P, F will use robust filter ver‐
45              sions: i.e., replace outliers (2.5 L1  scale  off  median)  with
46              median during filtering.
47              In  the  case of L|U it is possible that no data passes the ini‐
48              tial sign test; in that case the filter will return 0.0.
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OPTIONS

51       -D     increment is used when  series  is  NOT  equidistantly  sampled.
52              Then  increment  will  be  the  abscissae  resolution, i.e., all
53              abscissae will be  rounded  off  to  a  multiple  of  increment.
54              Alternatively, resample data with sample1d.
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56       -E     Include  Ends  of time series in output.  Default loses half the
57              filter-width of data at each end.
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59       -H     Input file(s) has Header record(s).  Number  of  header  records
60              can be changed by editing your .gmtdefaults4 file.  If used, GMT
61              default is 1 header record. Use -Hi if only  input  data  should
62              have  header  records  [Default will write out header records if
63              the input data have them]. Blank lines and lines starting with #
64              are always skipped.
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66       -I     To ignore values; If an input value equals ignore_val it will be
67              set to NaN.
68
69       -L     Checks for Lack of data condition.  If  input  data  has  a  gap
70              exceeding  width  then  no  output  will  be given at that point
71              [Default does not check Lack].
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73       -N     Sets number of columns in input and which  column  contains  the
74              independent  variable  (time).  The left-most column is # 0, the
75              right-most is # (n_cols - 1).  [Default is n_cols = 2,  t_col  =
76              0; i.e., file has t, f(t) pairs].
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78       -Q     assess Quality of output value by checking mean weight in convo‐
79              lution.  Enter q_factor between 0  and  1.   If  mean  weight  <
80              q_factor,  output  is suppressed at this point [Default does not
81              check Quality].
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83       -S     Checks symmetry of data about window  center.   Enter  a  factor
84              between  0  and  1.   If  (  (abs(n_left - n_right)) / (n_left +
85              n_right) ) > factor, then no output will be given at this  point
86              [Default does not check Symmetry].
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88       -T     Make  evenly spaced timesteps from start to stop by int [Default
89              uses input times].
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91       -V     Selects verbose mode, which will send progress reports to stderr
92              [Default runs "silently"].
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94       -bi    Selects binary input.  Append s for single precision [Default is
95              d  (double)].   Uppercase  S  or  D  will  force  byte-swapping.
96              Optionally,  append  ncol,  the number of columns in your binary
97              input file if it exceeds the columns needed by the program.   Or
98              append  c  if  the  input  file  is  netCDF.  Optionally, append
99              var1/var2/... to specify the variables to be read.
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101       -bo    Selects binary output.  Append s for single  precision  [Default
102              is  d  (double)].   Uppercase  S  or D will force byte-swapping.
103              Optionally, append ncol, the number of desired columns  in  your
104              binary output file.  [Default is same as input].
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106       -f     Special  formatting of input and/or output columns (time or geo‐
107              graphical data).  Specify i or o to  make  this  apply  only  to
108              input  or  output  [Default  applies to both].  Give one or more
109              columns (or column ranges) separated by commas.  Append T (abso‐
110              lute  calendar time), t (relative time in chosen TIME_UNIT since
111              TIME_EPOCH), x (longitude), y (latitude), or f (floating  point)
112              to  each  column or column range item.  Shorthand -f[i|o]g means
113              -f[i|o]0x,1y (geographic coordinates).
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ASCII FORMAT PRECISION

116       The ASCII output formats of numerical data are controlled by parameters
117       in  your  .gmtdefaults4  file.   Longitude  and  latitude are formatted
118       according to OUTPUT_DEGREE_FORMAT, whereas other values  are  formatted
119       according  to D_FORMAT.  Be aware that the format in effect can lead to
120       loss of precision in the output, which can  lead  to  various  problems
121       downstream.   If  you find the output is not written with enough preci‐
122       sion, consider switching to binary output (-bo if available) or specify
123       more decimals using the D_FORMAT setting.
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EXAMPLES

126       To filter the data set in the file cruise.gmtd containing evenly spaced
127       gravity, magnetics, topography, and distance (in m) with a 10 km Gauss‐
128       ian  filter,  removing outliers, and output a filtered value every 2 km
129       between 0 and 100 km:
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131       filter1d  cruise.gmtd  -T0/1.0e5/2000  -FG10000   -N4/3   -V   >   fil‐
132       tered_cruise.gmtd
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134       Data  along  track  often have uneven sampling and gaps which we do not
135       want to interpolate using sample1d.  To find the median depth in  a  50
136       km  window  every  25  km  along  the  track of cruise v3312, stored in
137       v3312.dt, checking for gaps of 10km and asymmetry of 0.3:
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139       filter1d v3312.dt -FM50 -T0/100000/25 -L10 -S0.3 > v3312_filt.dt
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SEE ALSO

142       GMT(1), sample1d(1)
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146GMT 4.3.1                         15 May 2008                      FILTER1D(1)
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