Author: bugman Date: Wed Jul 17 17:08:30 2013 New Revision: 20363 URL: http://svn.gna.org/viewcvs/relax?rev=20363&view=rev Log: Created the 'NS 2-site expanded' model target function. This is the numerical model for the 2-site Bloch-McConnell equations expanded using Maple by Nikolai Skrynnikov. It originates as optimization function number 5 from the fitting_main_kex.py script from Mathilde Lescanne, Paul Schanda, and Dominique Marion (see http://thread.gmane.org/gmane.science.nmr.relax.devel/4138, https://gna.org/task/?7712#comment2 and https://gna.org/support/download.php?file_id=18262). This commit follows step 4 of the relaxation dispersion model addition tutorial (http://thread.gmane.org/gmane.science.nmr.relax.devel/3907). Modified: branches/relax_disp/target_functions/relax_disp.py Modified: branches/relax_disp/target_functions/relax_disp.py URL: http://svn.gna.org/viewcvs/relax/branches/relax_disp/target_functions/relax_disp.py?rev=20363&r1=20362&r2=20363&view=diff ============================================================================== --- branches/relax_disp/target_functions/relax_disp.py (original) +++ branches/relax_disp/target_functions/relax_disp.py Wed Jul 17 17:08:30 2013 @@ -38,7 +38,7 @@ from lib.dispersion.ns_matrices import r180x_3d from lib.errors import RelaxError from target_functions.chi2 import chi2 -from specific_analyses.relax_disp.variables import MODEL_CR72, MODEL_CR72_RED, MODEL_DPL94, MODEL_IT99, MODEL_LIST_FULL, MODEL_LM63, MODEL_M61, MODEL_M61B, MODEL_NOREX, MODEL_NS_2SITE_3D, MODEL_NS_2SITE_3D_RED, MODEL_NS_2SITE_STAR, MODEL_NS_2SITE_STAR_RED, MODEL_R2EFF +from specific_analyses.relax_disp.variables import MODEL_CR72, MODEL_CR72_RED, MODEL_DPL94, MODEL_IT99, MODEL_LIST_FULL, MODEL_LM63, MODEL_M61, MODEL_M61B, MODEL_NOREX, MODEL_NS_2SITE_3D, MODEL_NS_2SITE_3D_RED, MODEL_NS_2SITE_EXPANDED, MODEL_NS_2SITE_STAR, MODEL_NS_2SITE_STAR_RED, MODEL_R2EFF class Dispersion: @@ -163,7 +163,7 @@ self.M0[0] = 0.5 # Some other data structures for the numerical solutions. - if model in [MODEL_NS_2SITE_3D_RED, MODEL_NS_2SITE_3D, MODEL_NS_2SITE_STAR_RED, MODEL_NS_2SITE_STAR]: + if model in [MODEL_NS_2SITE_3D_RED, MODEL_NS_2SITE_3D, MODEL_NS_2SITE_EXPANDED, MODEL_NS_2SITE_STAR_RED, MODEL_NS_2SITE_STAR]: # The tau_cpmg times and matrix exponential power array. self.tau_cpmg = zeros(self.num_disp_points, float64) self.power = zeros(self.num_disp_points, int16) @@ -195,6 +195,8 @@ self.func = self.func_ns_2site_3D_red if model == MODEL_NS_2SITE_3D: self.func = self.func_ns_2site_3D + if model == MODEL_NS_2SITE_EXPANDED: + self.func = self.func_ns_2site_expanded if model == MODEL_NS_2SITE_STAR: self.func = self.func_ns_2site_star if model == MODEL_NS_2SITE_STAR_RED: @@ -735,6 +737,58 @@ return self.calc_ns_2site_3D_chi2(R20A=R20, R20B=R20, dw=dw, pA=pA, kex=kex) + def func_ns_2site_expanded(self, params): + """Target function for the numerical solution for the 2-site Bloch-McConnell equations using the expanded notation. + + @param params: The vector of parameter values. + @type params: numpy rank-1 float array + @return: The chi-squared value. + @rtype: float + """ + + # Scaling. + if self.scaling_flag: + params = dot(params, self.scaling_matrix) + + # Unpack the parameter values. + R20 = params[:self.end_index[0]] + dw = params[self.end_index[0]:self.end_index[1]] + pA = params[self.end_index[1]] + kex = params[self.end_index[1]+1] + + # Once off parameter conversions. + pB = 1.0 - pA + k_AB = pA * kex + k_BA = pB * kex + + # Chi-squared initialisation. + chi2_sum = 0.0 + + # Loop over the spins. + for spin_index in range(self.num_spins): + # Loop over the spectrometer frequencies. + for frq_index in range(self.num_frq): + # The R20 index. + r20_index = frq_index + spin_index*self.num_frq + + # Convert dw from ppm to rad/s. + dw_frq = dw[spin_index] * self.frqs[spin_index, frq_index] + + # Back calculate the R2eff values. + r2eff_ns_2site_expanded(r20=R20[r20_index], pA=pA, dw=dw_frq, k_AB=k_AB, k_BA=k_BA, relax_time=self.relax_time, inv_relax_time=self.inv_relax_time, tcp=self.tau_cpmg, back_calc=self.back_calc[spin_index, frq_index], num_points=self.num_disp_points, num_cpmg=self.power) + + # For all missing data points, set the back-calculated value to the measured values so that it has no effect on the chi-squared value. + for point_index in range(self.num_disp_points): + if self.missing[spin_index, frq_index, point_index]: + self.back_calc[spin_index, frq_index, point_index] = self.values[spin_index, frq_index, point_index] + + # Calculate and return the chi-squared value. + chi2_sum += chi2(self.values[spin_index, frq_index], self.back_calc[spin_index, frq_index], self.errors[spin_index, frq_index]) + + # Return the total chi-squared value. + return chi2_sum + + def func_ns_2site_star(self, params): """Target function for the numerical solution for the 2-site Bloch-McConnell equations using complex conjugate matrices.