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Sven Czarnian
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external/include/GeographicLib/Gnomonic.hpp vendored Normal file
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/**
* \file Gnomonic.hpp
* \brief Header for GeographicLib::Gnomonic class
*
* Copyright (c) Charles Karney (2010-2020) <charles@karney.com> and licensed
* under the MIT/X11 License. For more information, see
* https://geographiclib.sourceforge.io/
**********************************************************************/
#if !defined(GEOGRAPHICLIB_GNOMONIC_HPP)
#define GEOGRAPHICLIB_GNOMONIC_HPP 1
#include <GeographicLib/Geodesic.hpp>
#include <GeographicLib/GeodesicLine.hpp>
#include <GeographicLib/Constants.hpp>
namespace GeographicLib {
/**
* \brief %Gnomonic projection
*
* %Gnomonic projection centered at an arbitrary position \e C on the
* ellipsoid. This projection is derived in Section 8 of
* - C. F. F. Karney,
* <a href="https://doi.org/10.1007/s00190-012-0578-z">
* Algorithms for geodesics</a>,
* J. Geodesy <b>87</b>, 43--55 (2013);
* DOI: <a href="https://doi.org/10.1007/s00190-012-0578-z">
* 10.1007/s00190-012-0578-z</a>;
* addenda:
* <a href="https://geographiclib.sourceforge.io/geod-addenda.html">
* geod-addenda.html</a>.
* .
* The projection of \e P is defined as follows: compute the geodesic line
* from \e C to \e P; compute the reduced length \e m12, geodesic scale \e
* M12, and &rho; = <i>m12</i>/\e M12; finally \e x = &rho; sin \e azi1; \e
* y = &rho; cos \e azi1, where \e azi1 is the azimuth of the geodesic at \e
* C. The Gnomonic::Forward and Gnomonic::Reverse methods also return the
* azimuth \e azi of the geodesic at \e P and reciprocal scale \e rk in the
* azimuthal direction. The scale in the radial direction if
* 1/<i>rk</i><sup>2</sup>.
*
* For a sphere, &rho; is reduces to \e a tan(<i>s12</i>/<i>a</i>), where \e
* s12 is the length of the geodesic from \e C to \e P, and the gnomonic
* projection has the property that all geodesics appear as straight lines.
* For an ellipsoid, this property holds only for geodesics interesting the
* centers. However geodesic segments close to the center are approximately
* straight.
*
* Consider a geodesic segment of length \e l. Let \e T be the point on the
* geodesic (extended if necessary) closest to \e C the center of the
* projection and \e t be the distance \e CT. To lowest order, the maximum
* deviation (as a true distance) of the corresponding gnomonic line segment
* (i.e., with the same end points) from the geodesic is<br>
* <br>
* (<i>K</i>(<i>T</i>) - <i>K</i>(<i>C</i>))
* <i>l</i><sup>2</sup> \e t / 32.<br>
* <br>
* where \e K is the Gaussian curvature.
*
* This result applies for any surface. For an ellipsoid of revolution,
* consider all geodesics whose end points are within a distance \e r of \e
* C. For a given \e r, the deviation is maximum when the latitude of \e C
* is 45&deg;, when endpoints are a distance \e r away, and when their
* azimuths from the center are &plusmn; 45&deg; or &plusmn; 135&deg;.
* To lowest order in \e r and the flattening \e f, the deviation is \e f
* (<i>r</i>/2<i>a</i>)<sup>3</sup> \e r.
*
* The conversions all take place using a Geodesic object (by default
* Geodesic::WGS84()). For more information on geodesics see \ref geodesic.
*
* \warning The definition of this projection for a sphere is
* standard. However, there is no standard for how it should be extended to
* an ellipsoid. The choices are:
* - Declare that the projection is undefined for an ellipsoid.
* - Project to a tangent plane from the center of the ellipsoid. This
* causes great ellipses to appear as straight lines in the projection;
* i.e., it generalizes the spherical great circle to a great ellipse.
* This was proposed by independently by Bowring and Williams in 1997.
* - Project to the conformal sphere with the constant of integration chosen
* so that the values of the latitude match for the center point and
* perform a central projection onto the plane tangent to the conformal
* sphere at the center point. This causes normal sections through the
* center point to appear as straight lines in the projection; i.e., it
* generalizes the spherical great circle to a normal section. This was
* proposed by I. G. Letoval'tsev, Generalization of the gnomonic
* projection for a spheroid and the principal geodetic problems involved
* in the alignment of surface routes, Geodesy and Aerophotography (5),
* 271--274 (1963).
* - The projection given here. This causes geodesics close to the center
* point to appear as straight lines in the projection; i.e., it
* generalizes the spherical great circle to a geodesic.
*
* Example of use:
* \include example-Gnomonic.cpp
*
* <a href="GeodesicProj.1.html">GeodesicProj</a> is a command-line utility
* providing access to the functionality of AzimuthalEquidistant, Gnomonic,
* and CassiniSoldner.
**********************************************************************/
class GEOGRAPHICLIB_EXPORT Gnomonic {
private:
typedef Math::real real;
real eps0_, eps_;
Geodesic _earth;
real _a, _f;
// numit_ increased from 10 to 20 to fix convergence failure with high
// precision (e.g., GEOGRAPHICLIB_DIGITS=2000) calculations. Reverse uses
// Newton's method which converges quadratically and so numit_ = 10 would
// normally be big enough. However, since the Geodesic class is based on a
// series it is of limited accuracy; in particular, the derivative rules
// used by Reverse only hold approximately. Consequently, after a few
// iterations, the convergence in the Reverse falls back to improvements in
// each step by a constant (albeit small) factor.
static const int numit_ = 20;
public:
/**
* Constructor for Gnomonic.
*
* @param[in] earth the Geodesic object to use for geodesic calculations.
* By default this uses the WGS84 ellipsoid.
**********************************************************************/
explicit Gnomonic(const Geodesic& earth = Geodesic::WGS84());
/**
* Forward projection, from geographic to gnomonic.
*
* @param[in] lat0 latitude of center point of projection (degrees).
* @param[in] lon0 longitude of center point of projection (degrees).
* @param[in] lat latitude of point (degrees).
* @param[in] lon longitude of point (degrees).
* @param[out] x easting of point (meters).
* @param[out] y northing of point (meters).
* @param[out] azi azimuth of geodesic at point (degrees).
* @param[out] rk reciprocal of azimuthal scale at point.
*
* \e lat0 and \e lat should be in the range [&minus;90&deg;, 90&deg;].
* The scale of the projection is 1/<i>rk</i><sup>2</sup> in the "radial"
* direction, \e azi clockwise from true north, and is 1/\e rk in the
* direction perpendicular to this. If the point lies "over the horizon",
* i.e., if \e rk &le; 0, then NaNs are returned for \e x and \e y (the
* correct values are returned for \e azi and \e rk). A call to Forward
* followed by a call to Reverse will return the original (\e lat, \e lon)
* (to within roundoff) provided the point in not over the horizon.
**********************************************************************/
void Forward(real lat0, real lon0, real lat, real lon,
real& x, real& y, real& azi, real& rk) const;
/**
* Reverse projection, from gnomonic to geographic.
*
* @param[in] lat0 latitude of center point of projection (degrees).
* @param[in] lon0 longitude of center point of projection (degrees).
* @param[in] x easting of point (meters).
* @param[in] y northing of point (meters).
* @param[out] lat latitude of point (degrees).
* @param[out] lon longitude of point (degrees).
* @param[out] azi azimuth of geodesic at point (degrees).
* @param[out] rk reciprocal of azimuthal scale at point.
*
* \e lat0 should be in the range [&minus;90&deg;, 90&deg;]. \e lat will
* be in the range [&minus;90&deg;, 90&deg;] and \e lon will be in the
* range [&minus;180&deg;, 180&deg;]. The scale of the projection is
* 1/<i>rk</i><sup>2</sup> in the "radial" direction, \e azi clockwise from
* true north, and is 1/\e rk in the direction perpendicular to this. Even
* though all inputs should return a valid \e lat and \e lon, it's possible
* that the procedure fails to converge for very large \e x or \e y; in
* this case NaNs are returned for all the output arguments. A call to
* Reverse followed by a call to Forward will return the original (\e x, \e
* y) (to roundoff).
**********************************************************************/
void Reverse(real lat0, real lon0, real x, real y,
real& lat, real& lon, real& azi, real& rk) const;
/**
* Gnomonic::Forward without returning the azimuth and scale.
**********************************************************************/
void Forward(real lat0, real lon0, real lat, real lon,
real& x, real& y) const {
real azi, rk;
Forward(lat0, lon0, lat, lon, x, y, azi, rk);
}
/**
* Gnomonic::Reverse without returning the azimuth and scale.
**********************************************************************/
void Reverse(real lat0, real lon0, real x, real y,
real& lat, real& lon) const {
real azi, rk;
Reverse(lat0, lon0, x, y, lat, lon, azi, rk);
}
/** \name Inspector functions
**********************************************************************/
///@{
/**
* @return \e a the equatorial radius of the ellipsoid (meters). This is
* the value inherited from the Geodesic object used in the constructor.
**********************************************************************/
Math::real EquatorialRadius() const { return _earth.EquatorialRadius(); }
/**
* @return \e f the flattening of the ellipsoid. This is the value
* inherited from the Geodesic object used in the constructor.
**********************************************************************/
Math::real Flattening() const { return _earth.Flattening(); }
/**
* \deprecated An old name for EquatorialRadius().
**********************************************************************/
GEOGRAPHICLIB_DEPRECATED("Use EquatorialRadius()")
Math::real MajorRadius() const { return EquatorialRadius(); }
///@}
};
} // namespace GeographicLib
#endif // GEOGRAPHICLIB_GNOMONIC_HPP