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lemma.h 14KB

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