gctl/lib/geometry/refellipsoid.h

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/********************************************************
*
*
*
*
*
*
* Geophysical Computational Tools & Library (GCTL)
*
* Copyright (c) 2023 Yi Zhang (yizhang-geo@zju.edu.cn)
*
* GCTL is distributed under a dual licensing scheme. You can redistribute
* it and/or modify it under the terms of the GNU Lesser General Public
* License as published by the Free Software Foundation, either version 2
* of the License, or (at your option) any later version. You should have
* received a copy of the GNU Lesser General Public License along with this
* program. If not, see <http://www.gnu.org/licenses/>.
*
* If the terms and conditions of the LGPL v.2. would prevent you from using
* the GCTL, please consider the option to obtain a commercial license for a
* fee. These licenses are offered by the GCTL's original author. As a rule,
* licenses are provided "as-is", unlimited in time for a one time fee. Please
* send corresponding requests to: yizhang-geo@zju.edu.cn. Please do not forget
* to include some description of your company and the realm of its activities.
* Also add information on how to contact you by electronic and paper mail.
******************************************************/
#ifndef _GCTL_REFELLIPSOID_H
#define _GCTL_REFELLIPSOID_H
#include "../core/macro.h"
#include "../core/exceptions.h"
#include "../maths/mathfunc.h"
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#include "point3c.h"
#include "point3s.h"
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namespace gctl
{
enum refellipsoid_type_e
{
// reference system named as the planet name represents a mean radius reference sphere
Earth,
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MagEarth,
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Moon,
Mars,
// Reference ellipsoids
WGS84,
Ardalan2010,
};
/**
* @brief Reference ellipsoid object. Predefined ellipsoids include
* Earth, Moon, Mars, WGS84 and Ardalan2010.
*
*/
class refellipsoid
{
public:
refellipsoid(/* args */);
refellipsoid(refellipsoid_type_e refellipsoid);
refellipsoid(double R, double r_or_alpha, bool is_alpha = false);
virtual ~refellipsoid();
/**
* @brief Initiate the reference ellipsoid using predefined parameters
*
* @param refellipsoid Predefined reference ellipsoid which includes Earth, Moon, Mars, WGS84 and Ardalan2010
*/
void set(refellipsoid_type_e refellipsoid);
/**
* @brief Initiate the reference ellipsoid using costumed parameters
*
* @param R Equator radius
* @param r_or_alpha Pole radius or the denominator of the flattening parameter
* @param is_flat Is the second paramter indicates the flattening parameter or not
*/
void set(double R, double r_or_flat, bool is_flat = false);
/**
* @brief Get the ellipsoidal radius at the inquiring latitude
*
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* @param geocentric_lati the inquiring latitude
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* @return ellipsoidal radius
*/
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double radius_at(double geocentric_lati);
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/**
* @brief Converts Geodetic coordinates to Spherical coordinates
*
* @param geodetic_lati Geodetic latitude
* @param geodetic_hei Height above the ellipsoid
* @param sph_lati Spherical latitude
* @param sph_rad Spherical radius
*/
void geodetic2spherical(double geodetic_lati, double geodetic_hei,
double& sph_lati, double& sph_rad);
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void spherical2geodetic(const point3ds& ps, double& geodetic_lon, double& geodetic_lati,
double& geodetic_hei, double eps = 1e-16, int cnt = 30);
/**
* @brief Convert xyz coordinates to Geodetic coodinates
*
* @param pc A point
* @param geodetic_lon Geodetic longitude
* @param geodetic_lati Geodetic latitude
* @param geodetic_hei Height above the ellipsoid
* @param eps solving precision
* @param cnt maximal iteration
*/
void xyz2geodetic(const point3dc& pc, double& geodetic_lon, double& geodetic_lati,
double& geodetic_hei, double eps = 1e-16, int cnt = 30);
void geodetic2xyz(double geodetic_lon, double geodetic_lati,
double geodetic_hei, point3dc& pc);
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private:
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double r_, R_, f_; // semi-minor, semi-major and flat rate
double e_;
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};
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};
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#endif // _GCTL_REFELLIPSOID_H