gctl/example/eemd_ex.cpp

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2024-09-10 15:45:07 +08:00
/********************************************************
*
*
*
*
*
*
* 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.
******************************************************/
/* Copyright 2013 Perttu Luukko
* This file is part of libeemd.
* libeemd is free software: you can redistribute it and/or modify
* it under the terms of the GNU General Public License as published by
* the Free Software Foundation, either version 3 of the License, or
* (at your option) any later version.
* libeemd is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details.
* You should have received a copy of the GNU General Public License
* along with libeemd. If not, see <http://www.gnu.org/licenses/>.
*/
#include "../lib/core.h"
#include "../lib/io.h"
#include "../lib/algorithm.h"
using namespace gctl;
const size_t ensemble_size = 250;
const unsigned int S_number = 4;
const unsigned int num_siftings = 50;
const double noise_strength = 0.2;
const unsigned long int rng_seed = 0;
std::string outfile = "eemd_example.out";
// An example signal to decompose
const size_t N = 1024;
static inline double input_signal(double x) {
const double omega = 2*GCTL_Pi/(N-1);
return sin(17*omega*x)+0.5*(1.0-exp(-0.002*x))*sin(51*omega*x+1);
}
int main(int argc, char const *argv[]) try
{
// Define input data
array<double> inp(N);
for (size_t i=0; i<N; i++)
{
inp[i] = input_signal((double)i);
}
// Run eemd
matrix<double> outp;
// This is just a warpper of the function eemd() from libeemd
// IMFs are stored in rows of the output matrix in the shape of M*N
eemd1d(inp, outp, 0, ensemble_size, noise_strength, S_number, num_siftings, rng_seed);
std::ofstream ofile;
open_outfile(ofile, outfile);
size_t M = outp.row_size();
for (size_t j=0; j<N; j++)
{
ofile << inp[j];
for (size_t i=0; i<M; i++)
{
ofile << " " << outp[i][j];
}
ofile << "\n";
}
ofile.close();
return 0;
}
catch(std::exception &e)
{
GCTL_ShowWhatError(e.what(), GCTL_ERROR_ERROR, 0, 0, 0);
}