GeographicLib 2.4

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Public Member Functions | Static Public Member Functions | List of all members
GeographicLib::DST Class Reference

Discrete sine transforms. More...

`#include <GeographicLib/DST.hpp>`

## Public Member Functions
| DST (int N=0)
void | reset (int N)
int | N () const
void | transform (std::function< real(real)> f, real F[]) const
void | refine (std::function< real(real)> f, real F[]) const

## Static Public Member Functions
static real | eval (real sinx, real cosx, const real F[], int N)
static real | integral (real sinx, real cosx, const real F[], int N)
static real | integral (real sinx, real cosx, real siny, real cosy, const real F[], int N)

## Detailed Description

Discrete sine transforms.

This decomposes periodic functions \( f(\sigma) \) (period \( 2\pi \)) which are odd about \( \sigma = 0 \) and even about \( \sigma = \frac12 \pi \) into a Fourier series

\[ f(\sigma) = \sum_{l=0}^\infty F_l \sin\bigl((2l+1)\sigma\bigr). \]

The first \( N \) components of \( F_l \), for \(0 \le l < N\) may be approximated by

\[ F_l = \frac2N \sum_{j=1}^{N} p_j f(\sigma_j) \sin\bigl((2l+1)\sigma_j\bigr), \]

where \( \sigma_j = j\pi/(2N) \) and \( p_j = \frac12 \) for \( j = N \) and \( 1 \) otherwise. \( F_l \) is a discrete sine transform of type DST-III and may be conveniently computed using the fast Fourier transform, FFT; this is implemented with the DST::transform method.

Having computed \( F_l \) based on \( N \) evaluations of \( f(\sigma) \) at \( \sigma_j = j\pi/(2N) \), it is possible to refine these transform values and add another \( N \) coefficients by evaluating \( f(\sigma) \) at \( (j-\frac12)\pi/(2N) \); this is implemented with the DST::refine method.

Here we compute FFTs using the kissfft package https://github.com/mborgerding/kissfft by Mark Borgerding.

Example of use:

// Example of using the GeographicLib::DST class
#include <iostream>
#include <exception>
#include <vector>
#include <GeographicLib/Math.hpp>
#include <GeographicLib/DST.hpp>
using namespace std;
using namespace GeographicLib;
class sawtooth {
private:
double _a;
public:
sawtooth(double a) : _a(a) {}
// only called for x in (0, pi/2]. DST assumes function is periodic, period
// 2*pi, is odd about 0, and is even about pi/2.
double operator()(double x) const { return _a * x; }
};
int main() {
try {
sawtooth f(Math::pi()/4);
DST dst;
int N = 5, K = 2*N;
vector<double> tx(N), txa(2*N);
dst.reset(N);
dst.transform(f, tx.data());
cout << "Transform of sawtooth based on " << N << " points\n"
<< "approx 1, -1/9, 1/25, -1/49, ...\n";
for (int i = 0; i < min(K,N); ++i) {
int j = (2*i+1)*(2*i+1)*(1-((i&1)<<1));
cout << i << " " << tx[i] << " " << tx[i]*j << "\n";
}
tx.resize(2*N);
dst.refine(f, tx.data());
cout << "Add another " << N << " points\n";
for (int i = 0; i < min(K,2*N); ++i) {
int j = (2*i+1)*(2*i+1)*(1-((i&1)<<1));
cout << i << " " << tx[i] << " " << tx[i]*j << "\n";
}
dst.reset(2*N);
dst.transform(f, txa.data());
cout << "Retransform of sawtooth based on " << 2*N << " points\n";
for (int i = 0; i < min(K,2*N); ++i) {
int j = (2*i+1)*(2*i+1)*(1-((i&1)<<1));
cout << i << " " << txa[i] << " " << txa[i]*j << "\n";
}
cout << "Table of values and integral\n";
for (int i = 0; i <= K; ++i) {
double x = i*Math::pi()/(2*K), sinx = sin(x), cosx = cos(x);
cout << x << " " << f(x) << " "
<< DST::eval(sinx, cosx, txa.data(), 2*N) << " "
<< DST::integral(sinx, cosx, txa.data(), 2*N) << "\n";
}
}
catch (const exception& e) {
cerr << "Caught exception: " << e.what() << "\n";
return 1;
}
}
main
int main(int argc, const char *const argv[])
Definition CartConvert.cpp:28
DST.hpp
Header for GeographicLib::DST class.
Math.hpp
Header for GeographicLib::Math class.
GeographicLib::DST
Discrete sine transforms.
Definition DST.hpp:63
GeographicLib::DST::reset
void reset(int N)
Definition DST.cpp:24
GeographicLib::DST::transform
void transform(std::function< real(real)> f, real F[]) const
Definition DST.cpp:79
GeographicLib::DST::refine
void refine(std::function< real(real)> f, real F[]) const
Definition DST.cpp:87
GeographicLib
Namespace for GeographicLib.
Definition Accumulator.cpp:12
std
Definition NearestNeighbor.hpp:806

Note
  The FFTW package https://www.fftw.org/ can also be used. However this is a more complicated dependency, its CMake support is broken, and it doesn't work with mpreals (GEOGRAPHICLIB_PRECISION = 5).

Definition at line 63 of file DST.hpp.

## Constructor & Destructor Documentation

## ◆ DST()

GeographicLib::DST::DST | ( | int | N = 0 | ) |

Constructor specifying the number of points to use.

Parameters

  [in] | N | the number of points to use.

Definition at line 19 of file DST.cpp.

## Member Function Documentation

## ◆ reset()

void GeographicLib::DST::reset | ( | int | N | ) |

Reset the given number of points.

Parameters

  [in] | N | the number of points to use.

Definition at line 24 of file DST.cpp.

References N().

Referenced by GeographicLib::GeodesicExact::GeodesicExact().

## ◆ N()

int GeographicLib::DST::N | ( |  | ) | const
| inline

Return the number of points.

Returns
  the number of points to use.

Definition at line 93 of file DST.hpp.

Referenced by eval(), integral(), integral(), and reset().

## ◆ transform()

void GeographicLib::DST::transform | ( | std::function< real(real)> | f,
|  | real | F[] ) const

Determine first N terms in the Fourier series

Parameters

  [in] | f | the function used for evaluation.
  [out] | F | the first N coefficients of the Fourier series.

The evaluates \( f(\sigma) \) at \( \sigma = (j + 1) \pi / (2 N) \) for integer \( j \in [0, N) \). F should be an array of length at least N.

Definition at line 79 of file DST.cpp.

References GeographicLib::Math::pi().

## ◆ refine()

void GeographicLib::DST::refine | ( | std::function< real(real)> | f,
|  | real | F[] ) const

Refine the Fourier series by doubling the number of points sampled

Parameters

  [in] | f | the function used for evaluation.
  [in,out] | F | on input the first N coefficents of the Fourier series; on output the refined transform based on 2N points, i.e., the first 2N coefficents.

The evaluates \( f(\sigma) \) at additional points \( \sigma = (j + \frac12) \pi / (2 N) \) for integer \( j \in [0, N) \), computes the DST-IV transform of these, and combines this with the input F to compute the 2N term DST-III discrete sine transform. This is equivalent to calling transform with twice the value of N but is more efficient, given that the N term coefficients are already known. See the example code above.

Definition at line 87 of file DST.cpp.

References GeographicLib::Math::pi().

## ◆ eval()

Math::real GeographicLib::DST::eval | ( | real | sinx,
|  | real | cosx,
|  | const real | F[],
|  | int | N )
| static

Evaluate the Fourier sum given the sine and cosine of the angle

Parameters

  [in] | sinx | sinσ.
  [in] | cosx | cosσ.
  [in] | F | the array of Fourier coefficients.
  [in] | N | the number of Fourier coefficients.

Returns
  the value of the Fourier sum.

Definition at line 95 of file DST.cpp.

References N().

## ◆ integral() [1/2]

Math::real GeographicLib::DST::integral | ( | real | sinx,
|  | real | cosx,
|  | const real | F[],
|  | int | N )
| static

Evaluate the integral of Fourier sum given the sine and cosine of the angle

Parameters

  [in] | sinx | sinσ.
  [in] | cosx | cosσ.
  [in] | F | the array of Fourier coefficients.
  [in] | N | the number of Fourier coefficients.

Returns
  the value of the integral.

The constant of integration is chosen so that the integral is zero at \( \sigma = \frac12\pi \).

Definition at line 112 of file DST.cpp.

References N().

Referenced by GeographicLib::GeodesicLineExact::GenPosition().

## ◆ integral() [2/2]

Math::real GeographicLib::DST::integral | ( | real | sinx,
|  | real | cosx,
|  | real | siny,
|  | real | cosy,
|  | const real | F[],
|  | int | N )
| static

Evaluate the definite integral of Fourier sum given the sines and cosines of the angles at the endpoints.

Parameters

  [in] | sinx | sinσ1.
  [in] | cosx | cosσ1.
  [in] | siny | sinσ2.
  [in] | cosy | cosσ2.
  [in] | F | the array of Fourier coefficients.
  [in] | N | the number of Fourier coefficients.

Returns
  the value of the integral.

The integral is evaluated between limits σ1 and σ2.

Definition at line 127 of file DST.cpp.

References N().

The documentation for this class was generated from the following files:

- DST.hpp
- DST.cpp