mailr7893 - in /branches/spectral_errors/prompt: relax_fit.py spectrum.py


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Posted by edward on October 21, 2008 - 17:25:
Author: bugman
Date: Tue Oct 21 17:25:06 2008
New Revision: 7893

URL: http://svn.gna.org/viewcvs/relax?rev=7893&view=rev
Log:
Shifted the relax_fit.mean_and_error() user function interface to 
spectrum.mean_and_error().


Modified:
    branches/spectral_errors/prompt/relax_fit.py
    branches/spectral_errors/prompt/spectrum.py

Modified: branches/spectral_errors/prompt/relax_fit.py
URL: 
http://svn.gna.org/viewcvs/relax/branches/spectral_errors/prompt/relax_fit.py?rev=7893&r1=7892&r2=7893&view=diff
==============================================================================
--- branches/spectral_errors/prompt/relax_fit.py (original)
+++ branches/spectral_errors/prompt/relax_fit.py Tue Oct 21 17:25:06 2008
@@ -40,60 +40,6 @@
 
         # Place relax in the class namespace.
         self.__relax__ = relax
-
-
-    def mean_and_error(self):
-        """Function for calculating the average intensity and standard 
deviation of all spectra.
-
-
-        Errors of individual spin at a single time point
-        ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-        The variance for a single spin at a single time point is calculated 
by the formula:
-
-        -----
-
-            sigma^2 =  sum({Ii - Iav}^2) / (n - 1) ,
-
-        -----
-
-        where sigma^2 is the variance, sigma is the standard deviation, n is 
the total number of
-        collected spectra for the time point and i is the corresponding 
index, Ii is the peak
-        intensity for spectrum i, Iav is the mean over all spectra, ie the 
sum of all peak
-        intensities divided by n.
-
-
-        Averaging of the errors
-        ~~~~~~~~~~~~~~~~~~~~~~~
-
-        As the value of n in the above equation is always very low, normally 
only a couple of
-        spectra are collected per time point, the variance of all spins is 
averaged for a single
-        time point.  Although this results in all spins having the same 
error, the accuracy of the
-        error estimate is significantly improved.
-
-
-        Errors across multiple time points
-        ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-
-        If all spectra are collected in duplicate (triplicate or higher 
number of spectra are
-        supported), the each time point will have its own error estimate.  
However, if there are
-        time points in the series which only consist of a single spectrum, 
then the variances of
-        replicated time points will be averaged.  Hence, for the entire 
experiment there will be a
-        single error value for all spins and for all time points.
-
-        A better approach rather than averaging across all time points would 
be to use a form of
-        interpolation as the errors across time points generally decreases 
for longer time periods.
-        This is currently not implemented.
-        """
-
-
-        # Function intro text.
-        if self.__relax__.interpreter.intro:
-            text = sys.ps3 + "relax_fit.mean_and_error()"
-            print text
-
-        # Execute the functional code.
-        relax_fit_obj.mean_and_error()
 
 
     def read(self, file=None, dir=None, relax_time=0.0, format='sparky', 
heteronuc='N', proton='HN', int_col=None):

Modified: branches/spectral_errors/prompt/spectrum.py
URL: 
http://svn.gna.org/viewcvs/relax/branches/spectral_errors/prompt/spectrum.py?rev=7893&r1=7892&r2=7893&view=diff
==============================================================================
--- branches/spectral_errors/prompt/spectrum.py (original)
+++ branches/spectral_errors/prompt/spectrum.py Tue Oct 21 17:25:06 2008
@@ -85,6 +85,60 @@
 
         # Execute the functional code.
         intensity.set_error(error=error, spectrum_id=spectrum_id, 
spin_id=spin_id)
+
+
+    def mean_and_error(self):
+        """Function for calculating the average intensity and standard 
deviation of all spectra.
+
+
+        Errors of individual spin at a single time point
+        ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+
+        The variance for a single spin at a single time point is calculated 
by the formula:
+
+        -----
+
+            sigma^2 =  sum({Ii - Iav}^2) / (n - 1) ,
+
+        -----
+
+        where sigma^2 is the variance, sigma is the standard deviation, n is 
the total number of
+        collected spectra for the time point and i is the corresponding 
index, Ii is the peak
+        intensity for spectrum i, Iav is the mean over all spectra, ie the 
sum of all peak
+        intensities divided by n.
+
+
+        Averaging of the errors
+        ~~~~~~~~~~~~~~~~~~~~~~~
+
+        As the value of n in the above equation is always very low, normally 
only a couple of
+        spectra are collected per time point, the variance of all spins is 
averaged for a single
+        time point.  Although this results in all spins having the same 
error, the accuracy of the
+        error estimate is significantly improved.
+
+
+        Errors across multiple time points
+        ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+
+        If all spectra are collected in duplicate (triplicate or higher 
number of spectra are
+        supported), the each time point will have its own error estimate.  
However, if there are
+        time points in the series which only consist of a single spectrum, 
then the variances of
+        replicated time points will be averaged.  Hence, for the entire 
experiment there will be a
+        single error value for all spins and for all time points.
+
+        A better approach rather than averaging across all time points would 
be to use a form of
+        interpolation as the errors across time points generally decreases 
for longer time periods.
+        This is currently not implemented.
+        """
+
+
+        # Function intro text.
+        if self.__relax__.interpreter.intro:
+            text = sys.ps3 + "relax_fit.mean_and_error()"
+            print text
+
+        # Execute the functional code.
+        relax_fit_obj.mean_and_error()
 
 
     def read_intensities(self, file=None, dir=None, spectrum_id=None, 
heteronuc='N', proton='HN', int_col=None, mol_name_col=None, 
res_num_col=None, res_name_col=None, spin_num_col=None, spin_name_col=None, 
sep=None):




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