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

* 1w6o_monomero *

CA distance fluctuations for 2405021119234077922

--- normal mode 7 ---

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
ASP 1065 1.01 ALA 1001 -1.29 PRO 1025

GLY 1066 1.38 SER 1002 -0.50 LYS 1127

ASN 1039 0.84 GLY 1003 -0.31 ALA 1051

SER 1038 0.63 LEU 1004 -0.35 PHE 1133

SER 1038 0.48 VAL 1005 -0.49 HIS 1052

CYS 1130 0.53 ALA 1006 -0.42 HIS 1052

CYS 1130 0.41 SER 1007 -0.42 HIS 1052

ALA 1001 0.34 ASN 1008 -0.36 HIS 1052

GLY 1103 0.27 LEU 1009 -0.29 HIS 1052

ALA 1001 0.22 ASN 1010 -0.24 HIS 1052

GLY 1103 0.23 LEU 1011 -0.21 LEU 1004

GLU 1105 0.20 LYS 1012 -0.20 ALA 1132

LYS 1107 0.17 PRO 1013 -0.29 ARG 1018

PHE 1106 0.27 GLY 1014 -0.39 ARG 1018

GLU 1105 0.35 GLU 1015 -0.38 ALA 1132

CYS 1088 0.36 LEU 1017 -0.28 ARG 1018

GLY 1103 0.34 ARG 1018 -0.41 THR 1090

ALA 1006 0.34 VAL 1019 -0.29 ALA 1001

ALA 1121 0.35 ARG 1020 -0.43 ALA 1001

ASN 1039 0.40 GLY 1021 -0.58 ALA 1001

GLY 1066 0.41 GLU 1022 -0.80 ALA 1001

GLY 1066 0.39 VAL 1023 -0.89 ALA 1001

GLY 1066 0.45 ALA 1024 -1.17 ALA 1001

GLY 1066 0.38 PRO 1025 -1.29 ALA 1001

GLY 1066 0.38 ASP 1026 -1.22 ALA 1001

GLY 1066 0.39 ALA 1027 -0.97 ALA 1001

ALA 1067 0.34 LYS 1028 -0.76 ALA 1001

ALA 1067 0.35 SER 1029 -0.55 ALA 1001

GLY 1066 0.43 PHE 1030 -0.41 ALA 1001

GLY 1066 0.39 VAL 1031 -0.35 HIS 1052

GLY 1066 0.33 LEU 1032 -0.30 HIS 1052

SER 1002 0.39 ASN 1033 -0.39 HIS 1052

SER 1002 0.35 LEU 1034 -0.29 HIS 1052

SER 1002 0.47 GLY 1035 -0.28 HIS 1052

ALA 1001 0.58 LYS 1036 -0.28 HIS 1052

ALA 1001 0.73 ASP 1037 -0.39 HIS 1052

SER 1002 0.97 SER 1038 -0.48 HIS 1052

SER 1002 1.22 ASN 1039 -0.32 HIS 1052

SER 1002 0.89 ASN 1040 -0.24 HIS 1052

SER 1002 0.70 LEU 1041 -0.24 HIS 1052

SER 1002 0.50 CYS 1042 -0.12 HIS 1052

SER 1002 0.40 LEU 1043 -0.15 HIS 1052

SER 1002 0.45 HIS 1044 -0.23 HIS 1052

SER 1002 0.20 PHE 1045 -0.17 HIS 1052

GLY 1069 0.19 ASN 1046 -0.23 VAL 1005

GLY 1066 0.14 PRO 1047 -0.41 ALA 1001

PHE 1049 0.15 ARG 1048 -0.47 ALA 1001

ARG 1048 0.15 PHE 1049 -0.65 ALA 1001

GLN 1080 0.15 ASN 1050 -0.61 ALA 1001

THR 1070 0.23 ALA 1051 -0.48 ALA 1001

THR 1070 0.21 HIS 1052 -0.49 VAL 1005

ALA 1075 0.25 GLY 1053 -0.41 ALA 1001

ALA 1075 0.26 ASP 1054 -0.43 ALA 1001

VAL 1076 0.25 ALA 1055 -0.55 ALA 1001

VAL 1076 0.17 ASN 1056 -0.56 ALA 1001

LYS 1107 0.20 THR 1057 -0.42 ALA 1001

LYS 1107 0.16 ILE 1058 -0.33 ALA 1001

LYS 1107 0.20 VAL 1059 -0.19 SER 1038

SER 1002 0.28 CYS 1060 -0.16 SER 1038

SER 1002 0.49 ASN 1061 -0.21 GLU 1074

SER 1002 0.65 SER 1062 -0.18 PHE 1106

SER 1002 0.93 LYS 1063 -0.18 GLN 1072

SER 1002 0.96 ASP 1064 -0.17 LEU 1112

SER 1002 1.15 ASP 1065 -0.21 LEU 1112

SER 1002 1.38 GLY 1066 -0.19 GLY 1053

SER 1002 1.14 ALA 1067 -0.19 GLU 1071

SER 1002 0.90 TRP 1068 -0.24 GLU 1071

SER 1002 0.72 GLY 1069 -0.22 ALA 1075

SER 1002 0.55 THR 1070 -0.28 ALA 1075

SER 1002 0.38 GLU 1071 -0.26 ARG 1073

SER 1002 0.25 GLN 1072 -0.30 GLU 1074

LYS 1107 0.32 ARG 1073 -0.26 GLU 1071

ASP 1054 0.24 GLU 1074 -0.30 GLN 1072

ASP 1134 0.28 ALA 1075 -0.35 ALA 1001

ASP 1134 0.28 VAL 1076 -0.43 ALA 1001

ASP 1134 0.24 PHE 1077 -0.52 ALA 1001

ASP 1134 0.23 PRO 1078 -0.58 ALA 1001

GLU 1086 0.19 PHE 1079 -0.66 ALA 1001

GLY 1066 0.21 GLN 1080 -0.81 ALA 1001

GLY 1066 0.29 PRO 1081 -0.98 ALA 1001

GLY 1066 0.34 GLY 1082 -1.09 ALA 1001

GLY 1066 0.29 SER 1083 -0.87 ALA 1001

GLY 1066 0.30 VAL 1084 -0.73 ALA 1001

GLY 1066 0.24 ALA 1085 -0.60 ALA 1001

ALA 1006 0.27 GLU 1086 -0.46 ALA 1001

ALA 1006 0.22 VAL 1087 -0.35 ALA 1001

ASP 1134 0.38 CYS 1088 -0.29 THR 1090

ASP 1134 0.34 ILE 1089 -0.21 LEU 1096

ASP 1134 0.31 THR 1090 -0.41 ARG 1018

LYS 1107 0.20 PHE 1091 -0.34 ARG 1018

ARG 1073 0.19 ASP 1092 -0.31 ARG 1018

SER 1002 0.23 GLN 1093 -0.24 ARG 1018

SER 1002 0.25 ALA 1094 -0.23 ARG 1018

ARG 1073 0.25 ASN 1095 -0.22 CYS 1088

ARG 1073 0.20 LEU 1096 -0.24 CYS 1088

ASP 1134 0.31 THR 1097 -0.25 CYS 1088

ASP 1134 0.36 VAL 1098 -0.21 VAL 1087

ASP 1134 0.47 LYS 1099 -0.29 ALA 1001

ASP 1134 0.36 LEU 1100 -0.40 ALA 1001

ARG 1018 0.32 PRO 1101 -0.51 ALA 1001

ASP 1134 0.40 ASP 1102 -0.51 ALA 1001

ASP 1134 0.53 GLY 1103 -0.40 ALA 1001

ASP 1134 0.46 TYR 1104 -0.36 ALA 1001

ASP 1134 0.47 GLU 1105 -0.27 ALA 1001

ASP 1134 0.35 PHE 1106 -0.26 PHE 1108

ARG 1073 0.32 LYS 1107 -0.24 PRO 1109

SER 1002 0.25 PHE 1108 -0.26 PHE 1106

SER 1002 0.33 PRO 1109 -0.25 PHE 1106

SER 1002 0.38 ASN 1110 -0.16 THR 1097

SER 1002 0.51 ARG 1111 -0.22 PHE 1106

SER 1002 0.58 LEU 1112 -0.21 ASP 1065

SER 1002 0.45 ASN 1113 -0.19 ASP 1065

SER 1002 0.41 LEU 1114 -0.19 ASP 1065

ALA 1001 0.33 GLU 1115 -0.17 ASP 1065

ALA 1001 0.28 ALA 1116 -0.16 HIS 1052

ALA 1001 0.28 ILE 1117 -0.22 HIS 1052

ALA 1001 0.36 ASN 1118 -0.30 HIS 1052

ALA 1001 0.39 TYR 1119 -0.38 HIS 1052

CYS 1130 0.33 MET 1120 -0.39 HIS 1052

SER 1038 0.45 ALA 1121 -0.47 HIS 1052

ASN 1039 0.57 ALA 1122 -0.36 HIS 1052

GLY 1066 0.72 ASP 1123 -0.36 VAL 1005

GLY 1066 0.65 GLY 1124 -0.39 ALA 1001

GLY 1066 0.55 ASP 1125 -0.75 ALA 1001

GLY 1066 0.50 PHE 1126 -0.65 ALA 1001

GLY 1066 0.59 LYS 1127 -0.67 ALA 1001

SER 1038 0.49 ILE 1128 -0.44 SER 1002

SER 1038 0.48 LYS 1129 -0.46 ALA 1001

ALA 1006 0.53 CYS 1130 -0.32 SER 1002

ALA 1006 0.44 VAL 1131 -0.33 SER 1002

GLY 1103 0.32 ALA 1132 -0.38 GLU 1015

GLY 1103 0.41 PHE 1133 -0.35 LEU 1004

GLY 1103 0.53 ASP 1134 -0.33 ALA 1132

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 7 ---

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

* 1w6o_monomero *