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6 gmtgravmag3d - Compute the gravity/magnetic effect of a body by the
7 method of Okabe
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10 gmtgravmag3d -Tpxyz_file[+m] -Tvvert_file OR -Tr|sraw_file [ -Cden‐
11 sity ] [ -D ] [ -Ethickness ] [ -Fxy_file ] [ -Goutputgrid ] [
12 -Hf_dec/f_dip/m_int/m_dec/m_dip ] [ -Lz_observation ] [ -Sradius ] [
13 -Zlevel ] [ -V[level] ] [ -fg]
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15 Note: No space is allowed between the option flag and the associated
16 arguments.
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19 gmtgravmag3d will compute the gravity or magnetic anomaly of a body
20 described by a set of triangles. The output can either be along a given
21 set of xy locations or on a grid. This method is not particularly fast
22 but allows computing the anomaly of arbitrarily complex shapes.
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25 -Cdensity
26 Sets body density in SI. This option is mutually exclusive with
27 -H.
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29 -Hf_dec/f_dip/m_int/m_dec/m_dip
30 Sets parameters for computing a magnetic anomaly. Use
31 f_dec/f_dip to set the geomagnetic declination/inclination in
32 degrees. m_int/m_dec/m_dip are the body magnetic intensity dec‐
33 lination and inclination.
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35 -Fxy_file
36 Provide locations where the anomaly will be computed. Note this
37 option is mutually exclusive with -G.
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39 -Goutgrid
40 Output the gravity or magnetic anomaly at nodes of this grid
41 file.
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43 -Rxmin/xmax/ymin/ymax[+r][+uunit] (more ...)
44 Specify the region of interest.
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46 -Tpxyz_file[+m] -Tvvert_file OR Tr|sraw_file
47 Gives names of xyz (-Tpxyz_file[+m]) and vertex (-Tvvert_file)
48 files defining a close surface. The file formats correspond to
49 the output of the triangulate program. The optional +m flag to
50 -Tp instructs the program that the xyzm file has four columns
51 and that the fourth column contains the magnetization intensity
52 (plus signal), which needs not to be constant. In this case the
53 third argument of the -H option is ignored. A raw format
54 (selected by the -Tr option) is a file with N rows (one per tri‐
55 angle) and 9 columns corresponding to the x,y,x coordinates of
56 each of the three vertex of each triangle. Alternatively, the
57 -Ts option indicates that the surface file is in the ASCII STL
58 (Stereo Lithographic) format. These two type of files are used
59 to provide a closed surface.
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62 -V[level] (more ...)
63 Select verbosity level [c].
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65 -E[thickness]
66 give layer thickness in m [Default = 0 m]. Use this option only
67 when the triangles describe a non-closed surface and you want
68 the anomaly of a constant thickness layer.
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70 -L[z_observation]
71 sets level of observation [Default = 0]. That is the height (z)
72 at which anomalies are computed.
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74 -Sradius
75 search radius in km. Triangle centroids that are further away
76 than radius from current output point will not be taken into
77 account. Use this option to speed up computation at expenses of
78 a less accurate result.
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80 -Z[level]
81 level of reference plane [Default = 0]. Use this option when the
82 triangles describe a non-closed surface and the volume is
83 defined from each triangle and this reference level. An example
84 will be the hater depth to compute a Bouguer anomaly.
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86 -fg Geographic grids (dimensions of longitude, latitude) will be
87 converted to meters via a "Flat Earth" approximation using the
88 current ellipsoid parameters.
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90 -^ or just -
91 Print a short message about the syntax of the command, then
92 exits (NOTE: on Windows just use -).
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94 -+ or just +
95 Print an extensive usage (help) message, including the explana‐
96 tion of any module-specific option (but not the GMT common
97 options), then exits.
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99 -? or no arguments
100 Print a complete usage (help) message, including the explanation
101 of all options, then exits.
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104 If the grid does not have meter as the horizontal unit, append +uunit
105 to the input file name to convert from the specified unit to meter. If
106 your grid is geographic, convert distances to meters by supplying -fg
107 instead.
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110 Suppose you ...
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112 gmt gmtgravmag3d ...
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115 gmt, grdgravmag3d, talwani2d, talwani3d
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118 Okabe, M., Analytical expressions for gravity anomalies due to polyhe‐
119 dral bodies and translation into magnetic anomalies, Geophysics, 44,
120 (1979), p 730-741.
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123 2019, P. Wessel, W. H. F. Smith, R. Scharroo, J. Luis, and F. Wobbe
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1285.4.5 Feb 24, 2019 GMTGRAVMAG3D(1)