mailRe: r23023 - /trunk/gui/analyses/auto_relax_disp.py


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Posted by Edward d'Auvergne on May 06, 2014 - 18:08:
Hi Troels,

Weird, 'B14' and 'B14 full' parameters look like the are reversed in
the diff.  But this is only because the diff cannot work out which
line changed :)  The change is good.

Cheers,

Edward



On 6 May 2014 17:34,  <tlinnet@xxxxxxxxxxxxx> wrote:
Author: tlinnet
Date: Tue May  6 17:34:20 2014
New Revision: 23023

URL: http://svn.gna.org/viewcvs/relax?rev=23023&view=rev
Log:
Added B14 and B14_FULL to the relax GUI.

sr #3154: (https://gna.org/support/?3154) Implementation of Baldwin (2014) 
B14 model - 2-site exact solution model for all time scales.

This follows the tutorial for adding relaxation dispersion models at:
http://wiki.nmr-relax.com/Tutorial_for_adding_relaxation_dispersion_models_to_relax#The_GUI


Modified:
    trunk/gui/analyses/auto_relax_disp.py

Modified: trunk/gui/analyses/auto_relax_disp.py
URL: 
http://svn.gna.org/viewcvs/relax/trunk/gui/analyses/auto_relax_disp.py?rev=23023&r1=23022&r2=23023&view=diff
==============================================================================
--- trunk/gui/analyses/auto_relax_disp.py       (original)
+++ trunk/gui/analyses/auto_relax_disp.py       Tue May  6 17:34:20 2014
@@ -48,7 +48,7 @@
 from pipe_control.mol_res_spin import exists_mol_res_spin_data, spin_loop
 from pipe_control.pipes import has_bundle, has_pipe
 from specific_analyses.relax_disp.data import has_cpmg_exp_type, 
has_r1rho_exp_type
-from specific_analyses.relax_disp.variables import MODEL_CR72, 
MODEL_CR72_FULL, MODEL_DPL94, MODEL_IT99, MODEL_LIST_CPMG, 
MODEL_LIST_R1RHO, MODEL_LM63, MODEL_LM63_3SITE, MODEL_M61, MODEL_M61B, 
MODEL_MMQ_CR72, MODEL_MP05, MODEL_NOREX, MODEL_NS_CPMG_2SITE_3D, 
MODEL_NS_CPMG_2SITE_3D_FULL, MODEL_NS_CPMG_2SITE_EXPANDED, 
MODEL_NS_CPMG_2SITE_STAR, MODEL_NS_CPMG_2SITE_STAR_FULL, 
MODEL_NS_MMQ_2SITE, MODEL_NS_MMQ_3SITE, MODEL_NS_MMQ_3SITE_LINEAR, 
MODEL_NS_R1RHO_2SITE, MODEL_NS_R1RHO_3SITE, MODEL_NS_R1RHO_3SITE_LINEAR, 
MODEL_R2EFF, MODEL_TAP03, MODEL_TP02, MODEL_TSMFK01
+from specific_analyses.relax_disp.variables import MODEL_B14, 
MODEL_B14_FULL, MODEL_CR72, MODEL_CR72_FULL, MODEL_DPL94, MODEL_IT99, 
MODEL_LIST_CPMG, MODEL_LIST_R1RHO, MODEL_LM63, MODEL_LM63_3SITE, MODEL_M61, 
MODEL_M61B, MODEL_MMQ_CR72, MODEL_MP05, MODEL_NOREX, 
MODEL_NS_CPMG_2SITE_3D, MODEL_NS_CPMG_2SITE_3D_FULL, 
MODEL_NS_CPMG_2SITE_EXPANDED, MODEL_NS_CPMG_2SITE_STAR, 
MODEL_NS_CPMG_2SITE_STAR_FULL, MODEL_NS_MMQ_2SITE, MODEL_NS_MMQ_3SITE, 
MODEL_NS_MMQ_3SITE_LINEAR, MODEL_NS_R1RHO_2SITE, MODEL_NS_R1RHO_3SITE, 
MODEL_NS_R1RHO_3SITE_LINEAR, MODEL_R2EFF, MODEL_TAP03, MODEL_TP02, 
MODEL_TSMFK01
 from status import Status; status = Status()


@@ -722,6 +722,8 @@
         MODEL_CR72_FULL,
         MODEL_IT99,
         MODEL_TSMFK01,
+        MODEL_B14,
+        MODEL_B14_FULL,
         MODEL_NS_CPMG_2SITE_EXPANDED,
         MODEL_NS_CPMG_2SITE_3D,
         MODEL_NS_CPMG_2SITE_3D_FULL,
@@ -755,6 +757,8 @@
         "{%s, ..., %s, %s, %s}" % (r2, phi_ex, padw2, kex),
         "{%s, ..., %s, k_AB}" % (r2a, dw),
         "{%s, ..., pA, %s, %s}" % (r2, dw, kex),
+        "{%s, %s, ..., pA, %s, %s}" % (r2a, r2b, dw, kex),
+        "{%s, ..., pA, %s, %s}" % (r2, dw, kex),
         "{%s, ..., pA, %s, %s}" % (r2, dw, kex),
         "{%s, %s, ..., pA, %s, %s}" % (r2a, r2b, dw, kex),
         "{%s, ..., pA, %s, %s}" % (r2, dw, kex),
@@ -786,6 +790,8 @@
         "The Carver and Richards (1972) 2-site equation for all time 
scales.",
         "The Ishima and Torchia (1999) 2-site model for all time scales 
with pA >> pB.",
         "The Tollinger et al. (2001) 2-site very-slow exchange model.",
+        "The Baldwin (2014) 2-site exact solution model for all time 
scales (with %s = %s)." % (r2a, r2b),
+        "The Baldwin (2014) 2-site exact solution model for all time 
scales.",
         "The 2-site numerical solution expanded using Maple by Nikolai 
Skrynnikov.",
         "The 2-site numerical solution using 3D magnetisation vectors 
(with %s = %s)." % (r2a, r2b),
         "The 2-site numerical solution using 3D magnetisation vectors.",


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