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GeographicLib
1.46
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Model of the earth's magnetic field. More...
#include <GeographicLib/MagneticModel.hpp>
Public Member Functions | |
Setting up the magnetic model | |
| MagneticModel (const std::string &name, const std::string &path="", const Geocentric &earth=Geocentric::WGS84()) | |
Inspector functions | |
| const std::string & | Description () const |
| const std::string & | DateTime () const |
| const std::string & | MagneticFile () const |
| const std::string & | MagneticModelName () const |
| const std::string & | MagneticModelDirectory () const |
| Math::real | MinHeight () const |
| Math::real | MaxHeight () const |
| Math::real | MinTime () const |
| Math::real | MaxTime () const |
| Math::real | MajorRadius () const |
| Math::real | Flattening () const |
Static Public Member Functions | |
| static std::string | DefaultMagneticPath () |
| static std::string | DefaultMagneticName () |
Compute the magnetic field | |
| void | operator() (real t, real lat, real lon, real h, real &Bx, real &By, real &Bz) const |
| void | operator() (real t, real lat, real lon, real h, real &Bx, real &By, real &Bz, real &Bxt, real &Byt, real &Bzt) const |
| MagneticCircle | Circle (real t, real lat, real h) const |
| static void | FieldComponents (real Bx, real By, real Bz, real &H, real &F, real &D, real &I) |
| static void | FieldComponents (real Bx, real By, real Bz, real Bxt, real Byt, real Bzt, real &H, real &F, real &D, real &I, real &Ht, real &Ft, real &Dt, real &It) |
Model of the earth's magnetic field.
Evaluate the earth's magnetic field according to a model. At present only internal magnetic fields are handled. These are due to the earth's code and crust; these vary slowly (over many years). Excluded are the effects of currents in the ionosphere and magnetosphere which have daily and annual variations.
See Magnetic models for details of how to install the magnetic models and the data format.
See
Example of use:
MagneticField is a command-line utility providing access to the functionality of MagneticModel and MagneticCircle.
Definition at line 63 of file MagneticModel.hpp.
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explicit |
Construct a magnetic model.
| [in] | name | the name of the model. |
| [in] | path | (optional) directory for data file. |
| [in] | earth | (optional) Geocentric object for converting coordinates; default Geocentric::WGS84(). |
| GeographicErr | if the data file cannot be found, is unreadable, or is corrupt. |
| std::bad_alloc | if the memory necessary for storing the model can't be allocated. |
A filename is formed by appending ".wmm" (World Magnetic Model) to the name. If path is specified (and is non-empty), then the file is loaded from directory, path. Otherwise the path is given by the DefaultMagneticPath().
This file contains the metadata which specifies the properties of the model. The coefficients for the spherical harmonic sums are obtained from a file obtained by appending ".cof" to metadata file (so the filename ends in ".wwm.cof").
The model is not tied to a particular ellipsoidal model of the earth. The final earth argument to the constructor specifies an ellipsoid to allow geodetic coordinates to the transformed into the spherical coordinates used in the spherical harmonic sum.
Definition at line 37 of file MagneticModel.cpp.
References DefaultMagneticPath(), GeographicLib::SphericalHarmonic::FULL, GeographicLib::Math::isfinite(), GeographicLib::Utility::ParseLine(), GeographicLib::SphericalEngine::coeff::readcoeffs(), and GeographicLib::SphericalHarmonic::SCHMIDT.
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inline |
Evaluate the components of the geomagnetic field.
| [in] | t | the time (years). |
| [in] | lat | latitude of the point (degrees). |
| [in] | lon | longitude of the point (degrees). |
| [in] | h | the height of the point above the ellipsoid (meters). |
| [out] | Bx | the easterly component of the magnetic field (nanotesla). |
| [out] | By | the northerly component of the magnetic field (nanotesla). |
| [out] | Bz | the vertical (up) component of the magnetic field (nanotesla). |
Definition at line 133 of file MagneticModel.hpp.
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inline |
Evaluate the components of the geomagnetic field and their time derivatives
| [in] | t | the time (years). |
| [in] | lat | latitude of the point (degrees). |
| [in] | lon | longitude of the point (degrees). |
| [in] | h | the height of the point above the ellipsoid (meters). |
| [out] | Bx | the easterly component of the magnetic field (nanotesla). |
| [out] | By | the northerly component of the magnetic field (nanotesla). |
| [out] | Bz | the vertical (up) component of the magnetic field (nanotesla). |
| [out] | Bxt | the rate of change of Bx (nT/yr). |
| [out] | Byt | the rate of change of By (nT/yr). |
| [out] | Bzt | the rate of change of Bz (nT/yr). |
Definition at line 155 of file MagneticModel.hpp.
| MagneticCircle GeographicLib::MagneticModel::Circle | ( | real | t, |
| real | lat, | ||
| real | h | ||
| ) | const |
Create a MagneticCircle object to allow the geomagnetic field at many points with constant lat, h, and t and varying lon to be computed efficiently.
| [in] | t | the time (years). |
| [in] | lat | latitude of the point (degrees). |
| [in] | h | the height of the point above the ellipsoid (meters). |
| std::bad_alloc | if the memory necessary for creating a MagneticCircle can't be allocated. |
If the field at several points on a circle of latitude need to be calculated then creating a MagneticCircle and using its member functions will be substantially faster, especially for high-degree models.
Definition at line 212 of file MagneticModel.cpp.
Referenced by main().
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inlinestatic |
Compute various quantities dependent on the magnetic field.
| [in] | Bx | the x (easterly) component of the magnetic field (nT). |
| [in] | By | the y (northerly) component of the magnetic field (nT). |
| [in] | Bz | the z (vertical, up positive) component of t |