diff --git a/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing.cpp b/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing.cpp
index 0c3e9b1ee2ab88965a3aefd5e1cb0106fa82377c..33863def3d3ccb651172167edcc3d1b4d9ab5069 100644
--- a/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing.cpp
+++ b/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing.cpp
@@ -1,6 +1,6 @@
 /*WIKI* 
 
-[[Image:GEM Focused.png|200px|thumb|right|Example of RAW GEM data focused across the 5 detector banks]] 
+[[Image:GEM_Focused.png|200px|thumb|right|Example of RAW GEM data focused across the 5 detector banks]]
 Given an InputWorkspace and a Grouping filename, the algorithm performs the following:
 # The calibration file is read and a map of corresponding udet-group is created.
 # The algorithm determine the X boundaries for each group as the upper and lower limits of all contributing detectors to this group and determine a logarithmic step that will ensure preserving the number of bins in the initial workspace.
diff --git a/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing2.cpp b/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing2.cpp
index 05075606d698fecc8a37365cffbb13a469be8db4..5bd8f0415be486560e6875efb7a8f74d8b7e4222 100644
--- a/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing2.cpp
+++ b/Code/Mantid/Framework/Algorithms/src/DiffractionFocussing2.cpp
@@ -1,6 +1,6 @@
 /*WIKI* 
 
-[[Image:GEM Focused.png|200px|thumb|right|Example of RAW GEM data focused across the 5 detector banks]] 
+[[Image:GEM_Focused.png|200px|thumb|right|Example of RAW GEM data focused across the 5 detector banks]]
 Given an InputWorkspace and a Grouping filename, the algorithm performs the following:
 # The calibration file is read and a map of corresponding udet-group is created.
 # The algorithm determine the X boundaries for each group as the upper and lower limits of all contributing detectors to this group and determine a logarithmic step that will ensure preserving the number of bins in the initial workspace.
diff --git a/Code/Mantid/Framework/Algorithms/src/GetEi.cpp b/Code/Mantid/Framework/Algorithms/src/GetEi.cpp
index 04062094e0f48190089ed23e6284ff63dbc48bc3..c3ff874dfd43253f51a197b13b7c8c21968823d2 100644
--- a/Code/Mantid/Framework/Algorithms/src/GetEi.cpp
+++ b/Code/Mantid/Framework/Algorithms/src/GetEi.cpp
@@ -13,7 +13,7 @@ Not all neutrons arrive at the monitors at the same time because their kinetic e
 # the mean of the X-values of the two half height points is the TOF arrival time of the neutrons
 
 The above process is illustrated on a peak is shown below in the image below
-[[File:monitorspect_getei.jpg|Monitor Peak|centre|618px]]
+[[File:Monitorspect_getei.jpg|Monitor Peak|centre|618px]]
 
 The distances between the monitors are read from the instrument definition file. It is assumed that the source and the monitors all lie on one line and that the monitors have the same delay time.
 
diff --git a/Code/Mantid/Framework/Algorithms/src/GetEi2.cpp b/Code/Mantid/Framework/Algorithms/src/GetEi2.cpp
index 12cdbbc4185a53f674e320a7e8ff3ff97ae9f613..6d4ac34fc0b46ed8bd5c6d46897d334d8cb722c2 100644
--- a/Code/Mantid/Framework/Algorithms/src/GetEi2.cpp
+++ b/Code/Mantid/Framework/Algorithms/src/GetEi2.cpp
@@ -13,7 +13,7 @@ Not all neutrons arrive at the monitors at the same time because their kinetic e
 # the mean of the X-values of the two half height points is the TOF arrival time of the neutrons
 
 The above process is illustrated on a peak is shown below in the image below
-[[File:monitorspect_getei.jpg|Monitor Peak|centre|618px]]
+[[File:Monitorspect_getei.jpg|Monitor Peak|centre|618px]]
 
 The distances between the monitors are read from the instrument definition file. It is assumed that the source and the monitors all lie on one line and that the monitors have the same delay time.
 
diff --git a/Code/Mantid/Framework/Algorithms/src/Q1D.cpp b/Code/Mantid/Framework/Algorithms/src/Q1D.cpp
index 2ce2fcca92e4499f958a6e203219823dc3ebd3de..7490f496f65f9892df12330257c877435716e629 100644
--- a/Code/Mantid/Framework/Algorithms/src/Q1D.cpp
+++ b/Code/Mantid/Framework/Algorithms/src/Q1D.cpp
@@ -15,7 +15,7 @@ where <math>m</math> is the particle's mass, <math>g</math> is the acceleration
 This [[Algorithm|algorithm]] takes a workspace of number of neutron counts against [[Units|wavelength]] and creates a workspace of cross section against Q. The output Q bins boundaries are defined by setting the property OutputBinning.
 
 Below is the formula used to calculate the cross section, <math>P_I(Q)</math>, for one bin in the output workspace whose bin number is denoted by I, when the input workspace has just one detector. Each bin is calculated from the sum of all input wavelength bins, n, that evaluate to the same Q using the formula for Q at the top of this page. In equations this relationship between the input bins and the output bins is represented by <math>n \supset I</math> and an example of a set of two bins is shown diagrammatically below.
-[[File:wav_Q_bins.png|Each Q bin contains the sum of many, one, or no wavelength bins|centre]]
+[[File:Wav_Q_bins.png|Each Q bin contains the sum of many, one, or no wavelength bins|centre]]
  
 In the equation the number of counts in the input spectrum number is denoted by <math>S(n)</math>, <math>N(n)</math> is the wavelength dependent correction and <math>\Omega</math> is the [[SolidAngle|solid angle]] of the detector
 
diff --git a/Code/Mantid/Framework/Algorithms/src/Q1D2.cpp b/Code/Mantid/Framework/Algorithms/src/Q1D2.cpp
index aa28103c81e478bdc4dcbd7e72c1c525d5f36c70..f1e83bbd091af835df7163cb3a12cd3abf8ddec0 100644
--- a/Code/Mantid/Framework/Algorithms/src/Q1D2.cpp
+++ b/Code/Mantid/Framework/Algorithms/src/Q1D2.cpp
@@ -15,7 +15,7 @@ where <math>m</math> is the particle's mass, <math>g</math> is the acceleration
 This [[Algorithm|algorithm]] takes a workspace of number of neutron counts against [[Units|wavelength]] and creates a workspace of cross section against Q. The output Q bins boundaries are defined by setting the property OutputBinning.
 
 Below is the formula used to calculate the cross section, <math>P_I(Q)</math>, for one bin in the output workspace whose bin number is denoted by I, when the input workspace has just one detector. Each bin is calculated from the sum of all input wavelength bins, n, that evaluate to the same Q using the formula for Q at the top of this page. In equations this relationship between the input bins and the output bins is represented by <math>n \supset I</math> and an example of a set of two bins is shown diagrammatically below.
-[[File:wav_Q_bins.png|Each Q bin contains the sum of many, one, or no wavelength bins|centre]]
+[[File:Wav_Q_bins.png|Each Q bin contains the sum of many, one, or no wavelength bins|centre]]
  
 In the equation the number of counts in the input spectrum number is denoted by <math>S(n)</math>, <math>N(n)</math> is the wavelength dependent correction and <math>\Omega</math> is the [[SolidAngle|solid angle]] of the detector
 
diff --git a/Code/Mantid/Framework/Algorithms/src/SassenaFFT.cpp b/Code/Mantid/Framework/Algorithms/src/SassenaFFT.cpp
index c72959ce530a8579f65ff6ca3f5a1aecda329d77..f8d778b71d3bdb0f37103f5021b3aec73e1e3def 100644
--- a/Code/Mantid/Framework/Algorithms/src/SassenaFFT.cpp
+++ b/Code/Mantid/Framework/Algorithms/src/SassenaFFT.cpp
@@ -18,7 +18,7 @@ Setting parameter FFTonlyRealPart to true will produce a transform on only the r
 
 Below are plots after application of SassenaFFT to <math>I(Q,t) = e^{-t^2/(2\sigma^2)} + i\cdot t \cdot e^{-t^2/(2\sigma^2)}</math> with <math>\sigma=1ps</math>. Real an imaginary parts are shown in panels (a) and (b). Note that <math>I(Q,t)*=I(Q,-t)</math>. If only <math>Re[I(Q,t)]</math> is transformed, the result is another Gaussian: <math>\sqrt{2\pi}\cdot e^{-E^2/(2\sigma'^2)}</math> with <math>\sigma'=4,136/(2\pi \sigma)</math> in units of <math>\mu</math>eV (panel (c)). If I(Q,t) is transformed, the result is a modulated Gaussian: <math>(1+\sigma' E)\sqrt{2\pi}\cdot e^{-E^2/(2\sigma'^2)}</math>(panel (d)).
 
-[[Image:sassenaFFTexample.jpg|center|x800px|alt=Application of SassenaFFT to a I(Q,t)]]
+[[Image:SassenaFFTexample.jpg|center|x800px|alt=Application of SassenaFFT to a I(Q,t)]]
 
  *WIKI*/