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  1. /* This file is part of Lemma, a geophysical modelling and inversion API */
  2. /* This Source Code Form is subject to the terms of the Mozilla Public
  3. * License, v. 2.0. If a copy of the MPL was not distributed with this
  4. * file, You can obtain one at http://mozilla.org/MPL/2.0/. */
  5. /**
  6. @file
  7. @author Trevor Irons
  8. @date 06/19/2009 09:12:20 AM The Birth of Lemma!
  9. @version $Id: lemma.h 203 2015-01-09 21:19:04Z tirons $
  10. **/
  11. // \image html lemma.png
  12. /** \mainpage Lemma is an ElectroMagnetics Modelling API
  13. \authors Trevor Irons and M. Andrew Kass and others
  14. Originally Lemma was intended as a recursive acronym standing for
  15. <B>L</B>emma is an <B>E</B>lectro<B>M</B>agnetics <B>M</B>odelling <B>A</B>PI.
  16. As the breadth of the project has expanded, the name has remained
  17. appropriate in a more liteal sense. Lemma is a flexible cross-platform
  18. library delivering an expressive API that can be used to easily create
  19. versatile programs. Lemma is not itself a program, instead it is a
  20. collection of building blocks to make applications. We retain this name because:
  21. - In mathematics a Lemma is a proven proposition which is used as a
  22. stepping stone to a larger result rather than as a statement in-and-of
  23. itself.
  24. - In addition to the electromagnetic modelling, some other facilities are
  25. provided such as numerical optimization and inversion capabilities. These
  26. tools are also considered stepping stones to final products.
  27. We feel that this is a partucularily approprate name, as Lemma's
  28. API can be leveraged create powerful applications such as forward
  29. modelling and inverting frequency and time-domain
  30. surveys of arbitrary survey design, sNMR surveys, CSAMT and more.
  31. \section Motivation
  32. Why another Geophysical EM project? For starters, there
  33. aren't that many quality open source packages out there. Those that do
  34. exist are generally specialized to perform a single task and extending
  35. them is a major undertaking. Lemma's approach is much different, by
  36. providing a set of general tools users can easily assemble applications
  37. that suite their needs.
  38. \section Capabilities Capabilities
  39. In the long term, we have many goals for this software project. Due to its
  40. design, Lemma can be built upon and extended easily. The initial aim is to
  41. provide flexible 1D and 3D EM modelling in the time and frequency domains.
  42. The project is still in beta, but we have made a lot of progress already.
  43. We will release our first non-beta release as soon as the following are
  44. supported.
  45. \subsection FDM Frequency-domain forward modelling
  46. Lemma was initially called EMMODFD: Electromagnetic Modelling in the Frequency
  47. Domain. As such this is the most mature area of Lemma.
  48. \par 1D
  49. Frequency domain solutions to electrical and magnetic dipoles can be computed
  50. quasi-analytically in 1D. Calculations can be made in or above the layered
  51. media, and complex electrical conductivity and magnetic susceptibility are
  52. supported according to the Cole-Cole model. Sources may be embdedded in the
  53. media or in the resisitive air layer. Lemma can also can compute fields due
  54. to arbitrarily shaped ungrounded wire loops, topography of the loops is also
  55. supported. Two separate approaches to solving the Hankel transform, one
  56. based on Anderson's digitial filtering technique, and another based on Gaussian
  57. quadrature.
  58. \par 3D
  59. A fast 3D solver that can modify the 1D results based
  60. on arbitrary electrical conductivity model is nearing completion.
  61. \par future work
  62. We are also planning on supporting grounded wires in the near future.
  63. \subsection TDM Time-domain forward modelling
  64. A 1D time-domain solution has been implemented that utilises both a
  65. dipole source as well as a wire loop. Currently, only one receiver is
  66. modelled at a time, but will be generalised. In addition, utilities
  67. to read in data files for modelling have been implemented.
  68. We would like to offer 3D time domain support, but this will not be
  69. provided before our first stable release.
  70. \subsection DataFormats Data Formats
  71. The EM community is plagued with myriad data formats. Often each equiptment
  72. manufacturer provides their own data format and interoperability is a
  73. constant struggle. We are working on a flexible data format based on the XML
  74. format that can be adapted to many types of data. The template for this
  75. format will be publically released and we hope it catches on in the community.
  76. At the least, it will provide a mechanism to compare datasets and datatypes
  77. within Lemma.
  78. \section Modules Modules
  79. Due to Lemma's design, it is easy to extend the platform. In some cases this
  80. extension results in adding functionality that is not directly related to
  81. ElectroMagnetics. The following modules utilise parts of Lemma to provide
  82. their functionality.
  83. \section Tutorials
  84. - \ref Tutorial - Basic intruduction to Lemma, including aquiring and
  85. compiling the code, class structure, and building your own
  86. applications.
  87. - \ref Extending Tutorial on how to extend Lemma.
  88. \section Development Development and design
  89. Ths package was initially developed by the Center for Gravity, Electrical, and
  90. Magnetic Studies (CGEM) at the Colorado School of Mines (CSM), the United
  91. States Geological Survey (USGS), and Broken Spoke Development, LLC. Where it drew
  92. on work by many others including Ki Ha Lee, and Walt Anderson. All new work and
  93. interfaces are written entirely in C++. Several small external projects are
  94. included, which are written in standard C, and FORTRAN 77. We adapt a
  95. modern, test driven, object oriented, C++ framework.
  96. More recent development has been undertaken at the University of Utah through the Energy
  97. and Geoscience Institute.
  98. \section Legalities
  99. \subsection Copyrights
  100. The following copyrights apply to the source.
  101. Most of the code was developed either by Trevor
  102. Copyright (C) 2008-2010 Trevor Irons <trevor.irons@lemmasoftware.org> or
  103. M. Andrew Kass Copyright (C) 2010 <mkass@usgs.gov>.
  104. The 1D EM solver was derived (but updated heavily) from a Fortran
  105. programme written by Ki Ha Lee in 1984. We have communicated with Ki Ha,
  106. and he assured us that this code is in the public domain.
  107. A Gaussian quadrature hankel transform originally written by Alan Chave was
  108. ported to C++. This code is in the public domain, and the source code was
  109. published in Geophysics.
  110. A digital filtering approach to the Hankel transform written by Walt
  111. Anderson was also rewritten for Lemma. The original Fortran code is also in
  112. the public domain.
  113. Please note that Ki Ha Lee and Walt Anderson had no part in this work, and
  114. the above should not be interpreted as any sort of endorsement by those
  115. parties.
  116. \subsection License
  117. This Source Code Form is subject to the terms of the Mozilla Public
  118. License, v. 2.0. If a copy of the MPL was not distributed with this
  119. file, You can obtain one at http://mozilla.org/MPL/2.0/.
  120. \section Contributing Suggestions and contributions
  121. We welcome contributions and suggestions. Feel free to email the development
  122. team at info@lemmasoftware.org.
  123. Under the terms of the MPL, if you modify a Lemma file, you are obligated to
  124. share those contributions back with the community.
  125. \section Useful Useful links
  126. - Home page https://lemmasoftware.org
  127. - Git repository https://git.lemmasoftware.org
  128. - Broken Spoke Develpment http://numericalgeo.com
  129. - CGEM at the Coloroado School of Mines http://geophysics.mines.edu/cgem/
  130. - EGI at the Eniversity of Utah http://egi.utah.edu/
  131. **/
  132. #pragma once
  133. #ifndef __LEMMA_H
  134. #define __LEMMA_H
  135. #include <LemmaConfig.h>
  136. // Include some basic stuff that will always be needed
  137. #include <iostream>
  138. #include <iomanip>
  139. #include <complex>
  140. #include <fstream>
  141. #include <string>
  142. #include <vector>
  143. #include <stdexcept>
  144. #include <sstream>
  145. #include <Eigen/Core>
  146. #include <cstddef>
  147. #include <Eigen/StdVector>
  148. #include <Eigen/Sparse>
  149. #include <unsupported/Eigen/FFT>
  150. //#include <unsupported/Eigen/SparseExtra>
  151. #include <Eigen/Geometry>
  152. /** \brief The only namespace used by Lemma
  153. *
  154. * \details The rational behind this namespace is that built-in
  155. * types should be used wherever possible, but not
  156. * not built-in names. This allows for code that is better
  157. * enacsulated and easier to modify. The typedefs and constants
  158. * specified here are defined so that
  159. * precision/inplimentation can easily be changed.
  160. * All floating precision types should be typedefed in this file
  161. * and should not be used natively within any code.
  162. * Lemma uses
  163. * the Eigen Matrix/Vector/Linear Algebra library.
  164. * <http://eigen.tuxfamily.org> and a lot of the namespece typedefs
  165. * are specifying Eigen types.
  166. */
  167. namespace Lemma {
  168. /// Real defines precision for the whole API, default is double
  169. #ifdef LEMMA_SINGLE_PRECISION
  170. typedef float Real;
  171. #else // ----- LEMMA_SINGLE_PRECISION -----
  172. typedef double Real;
  173. #endif // ----- not LEMMA_SINGLE_PRECISION -----
  174. /// Complex version of Real.
  175. typedef std::complex<Real> Complex;
  176. /// A 3 component Eigen vector of Reals
  177. typedef Eigen::Matrix<Real, 3, 1> Vector3r;
  178. /// A 3 X Dynamic Component Eigen matrix of Reals
  179. typedef Eigen::Matrix<Real, 3, Eigen::Dynamic> Vector3Xr;
  180. /// Variable length Eigen vector of Reals
  181. typedef Eigen::Matrix<Real, Eigen::Dynamic, 1> VectorXr;
  182. /// Variable length Eigen vector of integers (int)
  183. typedef Eigen::Matrix<int, Eigen::Dynamic, 1> VectorXi;
  184. /// Variable length Eigen vector of Complexes
  185. typedef Eigen::Matrix<Complex, Eigen::Dynamic, 1> VectorXcr;
  186. /// A 3 Component Eigen vector of Complexes
  187. typedef Eigen::Matrix<Complex, 3, 1> Vector3cr;
  188. /// A 3 X Dynamic Component Eigen matrix of Complexes
  189. typedef Eigen::Matrix<Complex, 3, Eigen::Dynamic> Vector3Xcr;
  190. /// Variable length Eigen Matrix of Reals
  191. typedef Eigen::Matrix<Real, Eigen::Dynamic, Eigen::Dynamic> MatrixXr;
  192. /// Variable length Eigen Matrix of ints
  193. typedef Eigen::Matrix<int, Eigen::Dynamic, Eigen::Dynamic> MatrixXi;
  194. /// Variable length Eigen vector of Complexes
  195. typedef Eigen::Matrix<Complex, Eigen::Dynamic, Eigen::Dynamic> MatrixXcr;
  196. ////////////////////////////////////////
  197. // Constants used across the programmes
  198. /// Restating the obvious, this is pi
  199. const Real PI = 4.0*atan(1.0);
  200. /// Permitivity of Free Space
  201. //const Real EPSILON0 = 8.854187817e-12;
  202. const Real EPSILON0 = 8.854187817e-12;
  203. /// Permeability of free space
  204. const Real MU0 = 4.*PI*1e-7;
  205. /// 1/4 of \f$ \pi\f$
  206. const Real QPI = .25/PI;
  207. /// Some functions will convert units from SI (standard) to Gauss
  208. /// This is because NMR calculations are much more natural in Gauss
  209. enum MAGUNITS {TESLA, NANOTESLA, GAUSS};
  210. /// Unit of temperature entered
  211. enum TEMPUNITS {CELCIUS, KELVIN};
  212. /// Unit of time entered
  213. enum TIMEUNITS {SEC, MILLISEC, MICROSEC, NANOSEC, PICOSEC};
  214. /// Unit of time entered
  215. enum FREQUENCYUNITS {HZ, KHZ, MHZ, GHZ};
  216. /// FEM coil relative orientations
  217. enum FEMCOILORIENTATION {COAXIAL, COPLANAR};
  218. /// General orientation relative to coordinate system
  219. enum ORIENTATION {X, Y, Z, NX, NY, NZ};
  220. /// Type of field
  221. enum FIELDTYPE {HFIELDREAL, HFIELDIMAG, EFIELDREAL, EFIELDIMAG};
  222. /// Compenent of vector field
  223. enum FIELDCOMPONENT {XCOMPONENT=0, YCOMPONENT=1, ZCOMPONENT=2};
  224. /// Spatial component of vector
  225. enum SPATIALCOORDINANT {XCOORD=0, YCOORD=1, ZCOORD=2};
  226. /** Evaluation method for Hankel integrals.
  227. * ANDERSON801 Walt Anderson's 801 point filter
  228. * CHAVE Alan Chave's gaussian quadrature integration method
  229. * FHTKEY201 Key's 201 point filter
  230. * FHTKEY201 Key's 101 point filter
  231. * FHTKEY51 Key's 51 point filter
  232. * QWEKEY Key's Gaussian quadrature integration method
  233. */
  234. enum HANKELTRANSFORMTYPE { ANDERSON801, CHAVE, FHTKEY201, FHTKEY101, FHTKEY51, QWEKEY };
  235. /** Enum is OK because these are the only physically possible sources.
  236. @param NOSOURCETYPE is default.
  237. @param ELECTRICDIPOLE is an electric dipole
  238. @param MAGNETICDIPOLE is a magnetic dipole
  239. */
  240. enum DipoleSourceType {NOSOURCETYPE, GROUNDEDELECTRICDIPOLE, UNGROUNDEDELECTRICDIPOLE, MAGNETICDIPOLE};
  241. /// Only three polarizations are supported. They may be summed to
  242. /// approximate others
  243. /// @param NOPOLARISATION is uninitialized, default value
  244. /// @param XPOLARISATION is a dipole oriented in the x direction
  245. /// @param YPOLARISATION is a dipole oriented in the y direction
  246. /// @param ZPOLARISATION is a dipole oriented in the z direction
  247. enum DipoleSourcePolarisation {NOPOLARISATION, XPOLARISATION,
  248. YPOLARISATION, ZPOLARISATION};
  249. /// The polarity may be either negative or positinve
  250. enum DipoleSourcePolarity {NEGATIVE, POSITIVE};
  251. /** The fields to make calculations on
  252. */
  253. enum FIELDCALCULATIONS {E, H, BOTH};
  254. /** Windowing function type
  255. */
  256. enum WINDOWTYPE { HAMMING, /*!< A hamming window */
  257. HANNING, /*!< A hanning window */
  258. RECTANGULAR /*!< Rectangular window */
  259. };
  260. }
  261. #endif // __Lemma_H