/******************************************************** * ██████╗ ██████╗████████╗██╗ * ██╔════╝ ██╔════╝╚══██╔══╝██║ * ██║ ███╗██║ ██║ ██║ * ██║ ██║██║ ██║ ██║ * ╚██████╔╝╚██████╗ ██║ ███████╗ * ╚═════╝ ╚═════╝ ╚═╝ ╚══════╝ * Geophysical Computational Tools & Library (GCTL) * * Copyright (c) 2022 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 . * * 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. ******************************************************/ #include "gctl/io.h" #include "gctl/geometry.h" #include "../lib/potential.h" using namespace gctl; int main(int argc, char const *argv[]) { mag_dipole md; md.M = 7.61365e+22; // 7.94e+22; md.n.set(point3dc(0.0, 0.0, 1.0)); point3ds op; point3dc B; for (int i = 0; i < 181; i++) { for (int j = 0; j < 361; j++) { op.lon = -180 + 1.0*j; op.lat = 90 - 1.0*i; op.rad = GCTL_Earth_Radius; B = magkernel_single(md, op); std::cout << op.lon << " " << op.lat << " " << B.x << " " << B.y << " " << B.z << " " << B.module() << "\n"; } } }