GeographicLib 2.1.2
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Local cartesian coordinates. More...
#include <GeographicLib/LocalCartesian.hpp>
Public Member Functions | |
LocalCartesian (real lat0, real lon0, real h0=0, const Geocentric &earth=Geocentric::WGS84()) | |
LocalCartesian (const Geocentric &earth=Geocentric::WGS84()) | |
void | Reset (real lat0, real lon0, real h0=0) |
void | Forward (real lat, real lon, real h, real &x, real &y, real &z) const |
void | Forward (real lat, real lon, real h, real &x, real &y, real &z, std::vector< real > &M) const |
void | Reverse (real x, real y, real z, real &lat, real &lon, real &h) const |
void | Reverse (real x, real y, real z, real &lat, real &lon, real &h, std::vector< real > &M) const |
Inspector functions | |
Math::real | LatitudeOrigin () const |
Math::real | LongitudeOrigin () const |
Math::real | HeightOrigin () const |
Math::real | EquatorialRadius () const |
Math::real | Flattening () const |
Local cartesian coordinates.
Convert between geodetic coordinates latitude = lat, longitude = lon, height = h (measured vertically from the surface of the ellipsoid) to local cartesian coordinates (x, y, z). The origin of local cartesian coordinate system is at lat = lat0, lon = lon0, h = h0. The z axis is normal to the ellipsoid; the y axis points due north. The plane z = - h0 is tangent to the ellipsoid.
The conversions all take place via geocentric coordinates using a Geocentric object (by default Geocentric::WGS84()).
Example of use:
CartConvert is a command-line utility providing access to the functionality of Geocentric and LocalCartesian.
Definition at line 38 of file LocalCartesian.hpp.
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Constructor setting the origin.
[in] | lat0 | latitude at origin (degrees). |
[in] | lon0 | longitude at origin (degrees). |
[in] | h0 | height above ellipsoid at origin (meters); default 0. |
[in] | earth | Geocentric object for the transformation; default Geocentric::WGS84(). |
lat0 should be in the range [−90°, 90°].
Definition at line 64 of file LocalCartesian.hpp.
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Default constructor.
[in] | earth | Geocentric object for the transformation; default Geocentric::WGS84(). |
Sets lat0 = 0, lon0 = 0, h0 = 0.
Definition at line 77 of file LocalCartesian.hpp.
void GeographicLib::LocalCartesian::Reset | ( | real | lat0, |
real | lon0, | ||
real | h0 = 0 |
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Reset the origin.
[in] | lat0 | latitude at origin (degrees). |
[in] | lon0 | longitude at origin (degrees). |
[in] | h0 | height above ellipsoid at origin (meters); default 0. |
lat0 should be in the range [−90°, 90°].
Definition at line 16 of file LocalCartesian.cpp.
References GeographicLib::Math::AngNormalize(), GeographicLib::Geocentric::Forward(), GeographicLib::Math::LatFix(), and GeographicLib::Math::sincosd().
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Convert from geodetic to local cartesian coordinates.
[in] | lat | latitude of point (degrees). |
[in] | lon | longitude of point (degrees). |
[in] | h | height of point above the ellipsoid (meters). |
[out] | x | local cartesian coordinate (meters). |
[out] | y | local cartesian coordinate (meters). |
[out] | z | local cartesian coordinate (meters). |
lat should be in the range [−90°, 90°].
Definition at line 104 of file LocalCartesian.hpp.
Referenced by main().
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Convert from geodetic to local cartesian coordinates and return rotation matrix.
[in] | lat | latitude of point (degrees). |
[in] | lon | longitude of point (degrees). |
[in] | h | height of point above the ellipsoid (meters). |
[out] | x | local cartesian coordinate (meters). |
[out] | y | local cartesian coordinate (meters). |
[out] | z | local cartesian coordinate (meters). |
[out] | M | if the length of the vector is 9, fill with the rotation matrix in row-major order. |
lat should be in the range [−90°, 90°].
Let v be a unit vector located at (lat, lon, h). We can express v as column vectors in one of two ways
Then we have v0 = M ⋅ v1.
Definition at line 135 of file LocalCartesian.hpp.
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Convert from local cartesian to geodetic coordinates.
[in] | x | local cartesian coordinate (meters). |
[in] | y | local cartesian coordinate (meters). |
[in] | z | local cartesian coordinate (meters). |
[out] | lat | latitude of point (degrees). |
[out] | lon | longitude of point (degrees). |
[out] | h | height of point above the ellipsoid (meters). |
In general, there are multiple solutions and the result which minimizes |h |is returned, i.e., (lat, lon) corresponds to the closest point on the ellipsoid. The value of lon returned is in the range [−180°, 180°].
Definition at line 161 of file LocalCartesian.hpp.
Referenced by main().
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Convert from local cartesian to geodetic coordinates and return rotation matrix.
[in] | x | local cartesian coordinate (meters). |
[in] | y | local cartesian coordinate (meters). |
[in] | z | local cartesian coordinate (meters). |
[out] | lat | latitude of point (degrees). |
[out] | lon | longitude of point (degrees). |
[out] | h | height of point above the ellipsoid (meters). |
[out] | M | if the length of the vector is 9, fill with the rotation matrix in row-major order. |
Let v be a unit vector located at (lat, lon, h). We can express v as column vectors in one of two ways
Then we have v1 = MT ⋅ v0, where MT is the transpose of M.
Definition at line 191 of file LocalCartesian.hpp.
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Definition at line 208 of file LocalCartesian.hpp.
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Definition at line 213 of file LocalCartesian.hpp.
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Definition at line 218 of file LocalCartesian.hpp.
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Definition at line 225 of file LocalCartesian.hpp.
References GeographicLib::Geocentric::EquatorialRadius().
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Definition at line 231 of file LocalCartesian.hpp.
References GeographicLib::Geocentric::Flattening().