EstimateMaterial.cpp 2.73 KB
#include "globals.h"
#define PI 3.14159

float CalculateError(float* E)
	//Calculate the error between the Reference Spectrum and the Simulated Spectrum
	float sumE = 0.0;
	int nVals = RefSpectrum[currentSpec].size();
	float nu;
	for(int i=0; i<nVals; i++)
		nu = RefSpectrum[currentSpec][i].nu;
		E[i] = RefSpectrum[currentSpec][i].A + nu * refSlope - SimSpectrum[i].A;
		sumE += E[i]*E[i];

	return sumE/nVals;

void EstimateK(float* E)
	int nVals = RefSpectrum[currentSpec].size();
	float nuStart = RefSpectrum[currentSpec].front().nu;
	float nuEnd = RefSpectrum[currentSpec].back().nu;

	float r = radius/10000.0;
	float nu;
	float dNu = (nuEnd - nuStart)/(nVals-1);
	float eScale;
	for(int i=0; i<nVals; i++)
		nu = nuStart + i*2;

		eScale = 1/(8*PI*r*nu);
		EtaK[i].A = EtaK[i].A + eScale * E[i];
		if(EtaK[i].A < 0.0) EtaK[i].A = 0.0;

void EstimateMaterial()
	/*This function estimates the material properties of a sphere based on the
	input spectrum RefSpectrum and the optical properties of the system.
	1) The material properties are stored in EtaK and EtaN
	2) The best fit is stored in SimSpectrum*/

	//initialize the material index of refraction

	//insert the default material properties
	SpecPair temp;
	for(int s=0; s<RefSpectrum[currentSpec].size(); s++)
		//the real part of the IR is the user-specified baseline IR = RefSpectrum[currentSpec][s].nu;
		temp.A = baseIR;
		//the imaginary part of the IR is zero absorbance
		temp.A = 0.0f;

	//allocate space to store the list of error values
	float* E = (float*)malloc(sizeof(float) * RefSpectrum[currentSpec].size());
	//copy the absorbance values into a linear array
	float* k = (float*)malloc(sizeof(float) * EtaK.size());
	float* n = (float*)malloc(sizeof(float) * EtaN.size());

	//iterate to solve for both n and k
	float sumE = 99999.9;
	int i=0;
	//clear the console
	while(sumE > minMSE && i < maxFitIter)
		//simulate a spectrum based on the current IR		

		//calculate the error term
		sumE = CalculateError(E);

		//estimate the new absorbance

		//use Kramers-Kronig to compute n
		for(int i=0; i<EtaK.size(); i++)
			k[i] = EtaK[i].A;
		cudaKramersKronig(n, k, EtaK.size(), EtaK.front().nu, EtaK.back().nu, baseIR);

		//copy the real part of the index of refraction into the vector
		for(int i=0; i<EtaK.size(); i++)
		{ =  EtaK[i].nu;
			temp.A = n[i];

		cout<<"    E = "<<sumE<<endl;
		//SaveSpectrum(n, nVals, "simNj.txt");
		//SaveSpectrum(k, nVals, "simKj.txt");
		//SaveSpectrum(simSpec, nVals, "simSpec.txt");