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gmtgravmag3d.rst 4.4 KB

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  1. .. index:: ! gmtgravmag3d
  2. .. include:: ../module_supplements_purpose.rst_
  3. ************
  4. gmtgravmag3d
  5. ************
  6. |gmtgravmag3d_purpose|
  7. Synopsis
  8. --------
  9. .. include:: ../../common_SYN_OPTs.rst_
  10. **gmt gravmag3d** |-T|\ **p**\ *xyz_file*\ [**+m**] |-T|\ **v**\ *vert_file* OR |-T|\ **r\|s**\ *raw_file*
  11. [ |-C|\ *density* ]
  12. [ |-D| ]
  13. [ |-E|\ *thickness* ]
  14. [ |-F|\ *xy_file* ]
  15. [ |-G|\ *outputgrid* ]
  16. [ |-H|\ *f_dec*/*f_dip*/*m_int*/*m_dec*/*m_dip* ]
  17. [ |-L|\ *z_observation* ]
  18. [ |-S|\ *radius* ]
  19. [ |-Z|\ *level* ]
  20. [ |SYN_OPT-V| ]
  21. [ **-fg**]
  22. [ |SYN_OPT--| ]
  23. |No-spaces|
  24. Description
  25. -----------
  26. **gravmag3d** will compute the gravity or magnetic anomaly of a body
  27. described by a set of triangles. The output can either be along a given
  28. set of xy locations or on a grid. This method is not particularly fast
  29. but allows computing the anomaly of arbitrarily complex shapes.
  30. Required Arguments
  31. ------------------
  32. .. _-C:
  33. **-C**\ *density*
  34. Sets body density in SI. This option is mutually exclusive with **-H**.
  35. .. _-H:
  36. **-H**\ *f_dec*/*f_dip*/*m_int*/*m_dec*/*m_dip*
  37. Sets parameters for computing a magnetic anomaly. Use
  38. *f_dec*/*f_dip* to set the geomagnetic declination/inclination in
  39. degrees. *m_int*/*m_dec*/*m_dip* are the body magnetic intensity
  40. declination and inclination.
  41. .. _-F:
  42. **-F**\ *xy_file*
  43. Provide locations where the anomaly will be computed. Note this
  44. option is mutually exclusive with **-G**.
  45. .. _-G:
  46. **-G**\ *outgrid*
  47. Output the gravity or magnetic anomaly at nodes of this grid file.
  48. .. _-R:
  49. .. |Add_-R| unicode:: 0x20 .. just an invisible code
  50. .. include:: ../../explain_-R.rst_
  51. .. _-T:
  52. **-Tp**\ *xyz_file*\ [**+m**] **-Tv**\ *vert_file* OR **Tr\|s**\ *raw_file*
  53. Gives names of xyz (**-Tp**\ *xyz_file*\ [**+m**]) and vertex (**-Tv**\ *vert_file*) files defining a close surface.
  54. The file formats correspond to the output of the :doc:`triangulate </triangulate>` program.
  55. The optional **+m** flag to **-Tp** instructs the program that the xyzm file
  56. has four columns and that the fourth column contains the magnetization intensity (plus signal),
  57. which needs not to be constant. In this case the third argument of the **-H** option is
  58. ignored. A *raw* format (selected by the **-Tr** option) is a file with N rows (one per triangle)
  59. and 9 columns corresponding to the x,y,x coordinates of each of the three vertex of each triangle.
  60. Alternatively, the **-Ts** option indicates that the surface file is in the ASCII STL (Stereo Lithographic) format.
  61. These two type of files are used to provide a closed surface.
  62. Optional Arguments
  63. ------------------
  64. .. _-V:
  65. .. |Add_-V| unicode:: 0x20 .. just an invisible code
  66. .. include:: ../../explain_-V.rst_
  67. .. _-E:
  68. **-E**\ [*thickness*]
  69. give layer thickness in m [Default = 0 m]. Use this option only when
  70. the triangles describe a non-closed surface and you want the anomaly
  71. of a constant thickness layer.
  72. .. _-L:
  73. **-L**\ [*z_observation*]
  74. sets level of observation [Default = 0]. That is the height (z) at
  75. which anomalies are computed.
  76. .. _-S:
  77. **-S**\ *radius*
  78. search radius in km. Triangle centroids that are further away than
  79. *radius* from current output point will not be taken into account.
  80. Use this option to speed up computation at expenses of a less
  81. accurate result.
  82. .. _-Z:
  83. **-Z**\ [*level*]
  84. level of reference plane [Default = 0]. Use this option when the
  85. triangles describe a non-closed surface and the volume is defined
  86. from each triangle and this reference level. An example will be the
  87. hater depth to compute a Bouguer anomaly.
  88. **-fg**
  89. Geographic grids (dimensions of longitude, latitude) will be converted to
  90. meters via a "Flat Earth" approximation using the current ellipsoid parameters.
  91. .. include:: ../../explain_help.rst_
  92. Grid Distance Units
  93. -------------------
  94. If the grid does not have meter as the horizontal unit, append **+u**\ *unit* to the input file name to convert from the
  95. specified unit to meter. If your grid is geographic, convert distances to meters by supplying **-fg** instead.
  96. Examples
  97. --------
  98. Suppose you ...
  99. ::
  100. gmt gravmag3d ...
  101. See Also
  102. --------
  103. :doc:`gmt </gmt>`, :doc:`grdgravmag3d`,
  104. :doc:`talwani2d </supplements/potential/talwani2d>`,
  105. :doc:`talwani3d </supplements/potential/talwani3d>`
  106. Reference
  107. ---------
  108. Okabe, M., Analytical expressions for gravity anomalies due to
  109. polyhedral bodies and translation into magnetic anomalies, *Geophysics*,
  110. 44, (1979), p 730-741.
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