Should you encounter any unexpected behaviour,
please let us know.

* 1w6o_monomero *

CA distance fluctuations for 2405021119234077922

--- normal mode 10 ---

This matrix displays the maximum distance fluctuations between all pairs of CA atoms and between the two extreme conformations that were computed for this mode (DQMIN/DQMAX). Distance increases are plotted in blue and decreases in red for the strongest 10% of the residue pair distance changes. Every pixel corresponds to a single residue. Grey lines are drawn every 10 residues, yellow lines every 100 residues (counting from the upper left corner).

The following table indicates for every residue the two corresponding residues with the strongest CA distance fluctuations.

[HELP on distance fluctuations]

GD ok

largest increase ref largest decrease
CYS 1130 0.77 ALA 1001 -1.02 HIS 1052

CYS 1130 0.93 SER 1002 -0.94 HIS 1052

CYS 1130 0.84 GLY 1003 -0.66 ASP 1125

VAL 1131 0.70 LEU 1004 -0.77 ASP 1125

ALA 1132 0.46 VAL 1005 -0.74 LYS 1127

ASP 1134 0.26 ALA 1006 -0.91 LYS 1127

ASP 1134 0.20 SER 1007 -0.74 LYS 1127

ASP 1037 0.34 ASN 1008 -0.69 LYS 1127

ALA 1001 0.24 LEU 1009 -0.67 LYS 1127

ALA 1001 0.18 ASN 1010 -0.59 LYS 1129

ALA 1001 0.22 LEU 1011 -0.52 LYS 1129

GLU 1105 0.19 LYS 1012 -0.43 LYS 1129

ALA 1075 0.25 PRO 1013 -0.32 LYS 1127

GLU 1105 0.31 GLY 1014 -0.26 CYS 1130

ALA 1001 0.32 GLU 1015 -0.33 CYS 1130

LEU 1004 0.46 LEU 1017 -0.31 VAL 1019

GLY 1003 0.58 ARG 1018 -0.30 GLU 1015

GLY 1003 0.69 VAL 1019 -0.36 LEU 1011

SER 1002 0.61 ARG 1020 -0.38 LEU 1009

SER 1002 0.58 GLY 1021 -0.52 ALA 1006

SER 1002 0.43 GLU 1022 -0.58 ALA 1006

SER 1002 0.19 VAL 1023 -0.51 ALA 1006

ASP 1102 0.12 ALA 1024 -0.64 LEU 1004

ASN 1056 0.22 PRO 1025 -0.58 LEU 1004

PHE 1049 0.26 ASP 1026 -0.62 LEU 1004

THR 1070 0.16 ALA 1027 -0.54 LEU 1004

THR 1070 0.21 LYS 1028 -0.59 GLY 1003

THR 1070 0.15 SER 1029 -0.58 GLY 1124

TRP 1068 0.04 PHE 1030 -0.35 ALA 1122

CYS 1130 0.07 VAL 1031 -0.27 ASN 1046

GLY 1003 0.19 LEU 1032 -0.33 LYS 1127

PHE 1133 0.09 ASN 1033 -0.39 LYS 1127

ASP 1134 0.12 LEU 1034 -0.46 LYS 1127

ASN 1008 0.18 GLY 1035 -0.45 LYS 1127

ASN 1008 0.29 LYS 1036 -0.49 LYS 1127

ASN 1008 0.34 ASP 1037 -0.60 SER 1002

ASN 1008 0.23 SER 1038 -0.80 SER 1002

ASN 1008 0.23 ASN 1039 -0.89 SER 1002

ASN 1008 0.23 ASN 1040 -0.67 SER 1002

ASN 1008 0.19 LEU 1041 -0.54 SER 1002

ASN 1008 0.16 CYS 1042 -0.41 SER 1002

GLY 1035 0.14 LEU 1043 -0.34 SER 1002

PHE 1133 0.09 HIS 1044 -0.43 SER 1002

LEU 1004 0.08 PHE 1045 -0.25 SER 1002

SER 1029 0.13 ASN 1046 -0.36 SER 1002

PHE 1108 0.18 PRO 1047 -0.30 ALA 1001

ASP 1026 0.22 ARG 1048 -0.50 ALA 1001

ASP 1026 0.26 PHE 1049 -0.49 ALA 1001

ASP 1026 0.25 ASN 1050 -0.71 ALA 1001

THR 1070 0.28 ALA 1051 -0.85 ALA 1001

THR 1070 0.32 HIS 1052 -1.02 ALA 1001

THR 1070 0.34 GLY 1053 -1.00 ALA 1001

GLN 1072 0.31 ASP 1054 -0.77 ALA 1001

GLN 1072 0.29 ALA 1055 -0.66 ALA 1001

PHE 1108 0.27 ASN 1056 -0.46 ALA 1001

PHE 1108 0.33 THR 1057 -0.46 ALA 1001

PHE 1108 0.30 ILE 1058 -0.34 ALA 1001

CYS 1060 0.28 VAL 1059 -0.45 SER 1002

VAL 1059 0.28 CYS 1060 -0.41 SER 1002

VAL 1059 0.19 ASN 1061 -0.51 SER 1002

ASN 1008 0.15 SER 1062 -0.55 SER 1002

ASN 1008 0.17 LYS 1063 -0.69 SER 1002

ASN 1008 0.19 ASP 1064 -0.69 SER 1002

ASN 1008 0.20 ASP 1065 -0.80 SER 1002

ASN 1008 0.19 GLY 1066 -0.93 SER 1002

ASN 1008 0.16 ALA 1067 -0.80 SER 1002

LYS 1028 0.14 TRP 1068 -0.75 SER 1002

GLY 1053 0.22 GLY 1069 -0.61 SER 1002

GLY 1053 0.34 THR 1070 -0.54 SER 1002

GLY 1053 0.28 GLU 1071 -0.57 SER 1002

PRO 1109 0.35 GLN 1072 -0.43 SER 1002

PRO 1109 0.41 ARG 1073 -0.43 ALA 1001

PHE 1108 0.35 GLU 1074 -0.31 ALA 1001

LYS 1107 0.42 ALA 1075 -0.31 ALA 1001

LYS 1107 0.32 VAL 1076 -0.21 ALA 1001

PHE 1106 0.29 PHE 1077 -0.20 ALA 1001

PHE 1106 0.24 PRO 1078 -0.12 ALA 1006

PHE 1106 0.21 PHE 1079 -0.22 ALA 1006

PRO 1025 0.20 GLN 1080 -0.31 ALA 1006

PRO 1025 0.22 PRO 1081 -0.41 ALA 1006

ASP 1102 0.18 GLY 1082 -0.46 ALA 1006

SER 1002 0.27 SER 1083 -0.40 ALA 1006

SER 1002 0.41 VAL 1084 -0.39 ALA 1006

SER 1002 0.37 ALA 1085 -0.27 LEU 1009

SER 1002 0.44 GLU 1086 -0.20 ASN 1010

GLY 1003 0.42 VAL 1087 -0.11 ASN 1010

GLY 1003 0.43 CYS 1088 -0.14 THR 1090

LEU 1004 0.35 ILE 1089 -0.17 LYS 1127

LEU 1004 0.27 THR 1090 -0.22 ARG 1018

PHE 1106 0.24 PHE 1091 -0.30 LYS 1127

ALA 1075 0.31 ASP 1092 -0.26 LYS 1127

ALA 1075 0.34 GLN 1093 -0.27 LYS 1127

ALA 1075 0.41 ALA 1094 -0.24 SER 1002

ALA 1075 0.39 ASN 1095 -0.20 SER 1002

ALA 1075 0.29 LEU 1096 -0.19 LYS 1127

ALA 1075 0.28 THR 1097 -0.11 PRO 1109

LEU 1004 0.25 VAL 1098 -0.10 THR 1070

GLY 1003 0.28 LYS 1099 -0.12 THR 1070

GLY 1003 0.24 LEU 1100 -0.08 ASN 1046

VAL 1084 0.30 PRO 1101 -0.08 ASN 1008

VAL 1084 0.35 ASP 1102 -0.09 VAL 1076

GLY 1003 0.26 GLY 1103 -0.14 TYR 1104

GLY 1014 0.24 TYR 1104 -0.14 GLN 1072

GLY 1014 0.31 GLU 1105 -0.19 THR 1070

ALA 1075 0.34 PHE 1106 -0.20 THR 1070

ALA 1075 0.42 LYS 1107 -0.20 PHE 1108

ARG 1073 0.41 PHE 1108 -0.23 SER 1002

ARG 1073 0.41 PRO 1109 -0.30 SER 1002

ARG 1073 0.33 ASN 1110 -0.34 SER 1002

ARG 1073 0.26 ARG 1111 -0.43 SER 1002

ARG 1073 0.22 LEU 1112 -0.47 SER 1002

ARG 1073 0.25 ASN 1113 -0.40 SER 1002

ALA 1075 0.20 LEU 1114 -0.37 SER 1002

ALA 1075 0.22 GLU 1115 -0.39 LYS 1127

ALA 1075 0.17 ALA 1116 -0.46 LYS 1127

THR 1090 0.17 ILE 1117 -0.51 LYS 1127

THR 1090 0.19 ASN 1118 -0.60 LYS 1127

ASP 1134 0.21 TYR 1119 -0.63 LYS 1127

PHE 1133 0.21 MET 1120 -0.70 LYS 1127

ALA 1132 0.23 ALA 1121 -0.67 LYS 1127

VAL 1019 0.35 ALA 1122 -0.58 ASP 1125

ILE 1128 0.55 ASP 1123 -0.64 HIS 1052

ILE 1128 0.22 GLY 1124 -0.62 ALA 1051

ASP 1102 0.07 ASP 1125 -0.77 LEU 1004

SER 1002 0.23 PHE 1126 -0.62 ALA 1006

SER 1002 0.55 LYS 1127 -0.91 ALA 1006

SER 1002 0.77 ILE 1128 -0.75 ALA 1006

SER 1002 0.92 LYS 1129 -0.68 ASN 1008

SER 1002 0.93 CYS 1130 -0.55 LEU 1009

GLY 1003 0.76 VAL 1131 -0.52 LYS 1129

ALA 1001 0.70 ALA 1132 -0.42 CYS 1130

ALA 1001 0.55 PHE 1133 -0.54 CYS 1130

ALA 1001 0.54 ASP 1134 -0.39 CYS 1130

If you find results from this site helpful for your research, please cite one of our papers:

K. Suhre & Y.H. Sanejouand, ElNemo: a normal mode web-server for protein movement analysis and the generation of templates for molecular replacement. Nucleic Acids Research, 32, W610-W614, 2004.
K. Suhre & Y.H. Sanejouand, On the potential of normal mode analysis for solving difficult molecular replacement problems. Acta Cryst. D vol.60, p796-799, 2004 © International Union of Crystallography.

elNémo is maintained by Yves-Henri Sanejouand.
It was developed by Karsten Suhre.
Between 2003 and 2014, it was hosted by IGS (Marseille).
Last modification: April 25th, 2023.

Should you encounter any unexpected behaviour, please let us know.

*** 1w6o_monomero ***

CA distance fluctuations for 2405021119234077922

--- normal mode 10 ---

Should you encounter any unexpected behaviour,
please let us know.

* 1w6o_monomero *