Changeset 87f8971 in sasview for sansmodels/src/sans/models/media/pd_help.html
- Timestamp:
- Dec 18, 2012 2:27:07 PM (12 years ago)
- Branches:
- master, ESS_GUI, ESS_GUI_Docs, ESS_GUI_batch_fitting, ESS_GUI_bumps_abstraction, ESS_GUI_iss1116, ESS_GUI_iss879, ESS_GUI_iss959, ESS_GUI_opencl, ESS_GUI_ordering, ESS_GUI_sync_sascalc, costrafo411, magnetic_scatt, release-4.1.1, release-4.1.2, release-4.2.2, release_4.0.1, ticket-1009, ticket-1094-headless, ticket-1242-2d-resolution, ticket-1243, ticket-1249, ticket885, unittest-saveload
- Children:
- 9714ff5
- Parents:
- 5b07138
- File:
-
- 1 edited
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sansmodels/src/sans/models/media/pd_help.html
r318b5bbb r87f8971 36 36 <p> </p> 37 37 <p><a name="Rectangular"><h4>Rectangular distribution</a></h4></p> 38 <p><img src=" ./img/pd_image001.png"></p>38 <p><img src="img/pd_image001.png"></p> 39 39 <p> </p> 40 40 <p>The x<sub>mean</sub> is the mean … … 43 43 the half width <i>w</i> are different.</p> 44 44 <p>The standard deviation is </p> 45 <p><img src=" ./img/pd_image002.png"></p>45 <p><img src="img/pd_image002.png"></p> 46 46 <p> </p> 47 47 <p>The PD (polydispersity) is </p> 48 <p><img src=" ./img/pd_image003.png"></p>48 <p><img src="img/pd_image003.png"></p> 49 49 <p> </p> 50 50 <p><img width=511 height=270 51 id="Picture 1" src=" ./img/pd_image004.jpg" alt=flat.gif></p>51 id="Picture 1" src="img/pd_image004.jpg" alt=flat.gif></p> 52 52 <p> </p> 53 53 <p> </p> … … 86 86 <p> </p> 87 87 88 <p><img src=" ./img/pd_image005.png"></p>88 <p><img src="img/pd_image005.png"></p> 89 89 90 90 <p> </p> … … 98 98 <p>The PD (polydispersity) is </p> 99 99 100 <p><img src=" ./img/pd_image003.png"></p>100 <p><img src="img/pd_image003.png"></p> 101 101 102 102 <p> </p> 103 103 104 104 <p><img width=518 height=275 105 id="Picture 2" src=" ./img/pd_image006.jpg" alt=gauss.gif></p>105 id="Picture 2" src="img/pd_image006.jpg" alt=gauss.gif></p> 106 106 107 107 <p> </p> … … 111 111 <p> </p> 112 112 113 <p><img src=" ./img/pd_image007.png"></p>113 <p><img src="img/pd_image007.png"></p> 114 114 115 115 <p> </p> … … 126 126 by σ,</p> 127 127 128 <p><img src=" ./img/pd_image008.png"></p>128 <p><img src="img/pd_image008.png"></p> 129 129 130 130 <p> </p> … … 132 132 <p>For the angular distribution,</p> 133 133 134 <p><img src=" ./img/pd_image009.png"></p>134 <p><img src="img/pd_image009.png"></p> 135 135 136 136 <p> </p> … … 144 144 145 145 <p><img width=450 height=239 146 id="Picture 7" src=" ./img/pd_image010.jpg" alt=lognormal.gif></p>146 id="Picture 7" src="img/pd_image010.jpg" alt=lognormal.gif></p> 147 147 148 148 <p> </p> … … 158 158 <p> </p> 159 159 160 <p><img src=" ./img/pd_image011.png"></p>160 <p><img src="img/pd_image011.png"></p> 161 161 162 162 <p> </p> … … 170 170 171 171 <p>The PD (polydispersity) is </p> 172 <p'><img src=" ./img/pd_image012.png"></p>172 <p'><img src="img/pd_image012.png"></p> 173 173 <p>Note that the higher PD (polydispersity) 174 174 might need higher values of Npts and Nsigmas. For example, at PD = 0.7 and radisus = 60 A, … … 176 176 <p/> 177 177 <p><img width=438 height=232 178 id="Picture 4" src=" ./img/pd_image013.jpg" alt=schulz.gif></p>178 id="Picture 4" src="img/pd_image013.jpg" alt=schulz.gif></p> 179 179 180 180 </div>
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