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***  Ahmad Khan  ***

CA distance fluctuations for 2603140834172769745

---  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 increasereflargest decrease
ARG 122 0.19 GLY 6 -0.21 LEU 154
ARG 122 0.21 PHE 7 -0.10 LYS 155
ARG 122 0.22 LEU 8 -0.09 LEU 154
LYS 42 0.21 GLU 9 -0.13 LEU 154
LYS 42 0.25 LEU 10 -0.12 ALA 58
LYS 42 0.33 GLU 11 -0.14 ALA 58
LYS 42 0.35 ARG 12 -0.13 ALA 58
LYS 42 0.34 SER 13 -0.15 ALA 58
LYS 42 0.42 SER 14 -0.19 ALA 58
LYS 42 0.42 GLY 15 -0.25 GLU 168
LYS 42 0.36 LYS 16 -0.32 ALA 58
ASN 49 0.29 LEU 17 -0.27 PRO 57
LYS 42 0.27 GLU 18 -0.21 SER 33
LYS 42 0.27 TRP 19 -0.17 ALA 58
ASN 49 0.22 SER 20 -0.18 SER 33
ASN 49 0.21 ALA 21 -0.24 SER 33
PRO 41 0.18 ILE 22 -0.17 SER 33
PRO 41 0.16 LEU 23 -0.12 SER 33
ASN 49 0.16 GLN 24 -0.21 SER 33
ASN 49 0.15 LYS 25 -0.18 ALA 134
ALA 121 0.24 ALA 27 -0.12 ILE 22
ALA 121 0.21 SER 28 -0.20 ALA 134
ALA 121 0.22 ASP 29 -0.16 ALA 134
ALA 121 0.28 LEU 30 -0.10 ASP 43
ALA 121 0.28 GLY 31 -0.16 GLU 139
ALA 121 0.27 PHE 32 -0.16 ALA 21
ALA 121 0.19 SER 33 -0.24 ALA 21
ALA 121 0.18 LYS 34 -0.19 LEU 17
ALA 121 0.19 ILE 35 -0.16 ASP 43
ALA 121 0.15 LEU 36 -0.18 ALA 166
ALA 121 0.14 PHE 37 -0.17 ALA 166
ASP 46 0.12 GLY 38 -0.21 ALA 58
GLY 15 0.17 LEU 39 -0.23 ALA 58
GLY 15 0.26 LEU 40 -0.40 ARG 122
ALA 166 0.43 PRO 41 -0.68 ARG 122
PHE 167 0.77 LYS 42 -0.45 SER 44
GLU 168 0.53 ASP 43 -0.81 THR 80
GLY 15 0.32 SER 44 -0.45 LYS 42
GLY 15 0.26 GLN 45 -0.52 ASP 43
GLY 15 0.27 ASP 46 -0.38 ARG 122
LEU 17 0.20 TYR 47 -0.40 ASP 43
LEU 17 0.22 GLU 48 -0.34 ARG 122
LEU 17 0.29 ASN 49 -0.43 ARG 122
LEU 17 0.23 ALA 50 -0.39 ARG 122
LYS 16 0.24 PHE 51 -0.38 ALA 58
ASN 49 0.22 ILE 52 -0.39 ALA 166
ASN 49 0.23 VAL 53 -0.28 ALA 58
ASN 49 0.18 GLY 54 -0.22 GLU 168
GLU 48 0.13 ASN 55 -0.23 LEU 17
SER 28 0.10 TYR 56 -0.25 ALA 166
SER 33 0.14 PRO 57 -0.31 ALA 166
SER 33 0.11 ALA 58 -0.42 ALA 166
ALA 108 0.12 ALA 59 -0.36 GLU 168
SER 33 0.08 TRP 60 -0.28 ALA 166
ASN 55 0.11 ARG 61 -0.31 ALA 166
ASN 55 0.09 GLU 62 -0.37 PHE 167
SER 28 0.07 HIS 63 -0.27 PHE 167
ASN 55 0.06 TYR 64 -0.31 ASP 43
ASN 55 0.10 ASP 65 -0.31 ASP 43
ASN 55 0.09 ARG 66 -0.30 ARG 122
LYS 25 0.06 ALA 67 -0.30 ASP 43
LEU 17 0.10 GLY 68 -0.36 ASP 43
ALA 121 0.12 TYR 69 -0.39 ASP 43
ALA 121 0.15 ALA 70 -0.47 ASP 43
ALA 121 0.18 ARG 71 -0.49 ASP 43
ALA 121 0.23 VAL 72 -0.42 ASP 43
ALA 121 0.27 ASP 73 -0.43 ASP 43
ALA 121 0.39 PRO 74 -0.44 ASP 43
ALA 121 0.43 THR 75 -0.45 ASP 43
ALA 121 0.35 VAL 76 -0.54 ASP 43
ALA 121 0.39 SER 77 -0.61 ASP 43
ALA 121 0.51 HIS 78 -0.57 ASP 43
ALA 121 0.54 CYS 79 -0.59 ASP 43
ALA 121 0.46 THR 80 -0.81 ASP 43
ALA 121 0.56 GLN 81 -0.68 ASP 43
ALA 121 0.74 SER 82 -0.54 ASP 43
ALA 121 0.96 VAL 83 -0.43 ASP 43
ALA 121 0.83 LEU 84 -0.38 ASP 43
ALA 121 0.70 PRO 85 -0.34 ASP 43
ALA 121 0.60 ILE 86 -0.36 ASP 43
ALA 121 0.53 PHE 87 -0.30 ASP 43
ALA 121 0.44 TRP 88 -0.30 ASP 43
ALA 121 0.46 GLU 89 -0.28 ASP 43
ALA 121 0.40 PRO 90 -0.27 ASP 43
ALA 121 0.46 SER 91 -0.27 ASP 43
ALA 121 0.47 ILE 92 -0.32 ASP 43
ALA 121 0.38 TYR 93 -0.31 ASP 43
ALA 121 0.40 GLN 94 -0.28 ASP 43
ALA 121 0.34 THR 95 -0.28 ASP 43
ALA 121 0.28 ARG 96 -0.26 ASP 43
ALA 121 0.23 LYS 97 -0.31 ASP 43
ALA 121 0.28 GLN 98 -0.33 ASP 43
ALA 121 0.28 HIS 99 -0.28 ASP 43
ALA 121 0.20 GLU 100 -0.28 ASP 43
ALA 121 0.21 PHE 101 -0.31 ASP 43
ALA 121 0.26 PHE 102 -0.29 ASP 43
ALA 121 0.22 GLU 103 -0.26 ASP 43
ALA 121 0.16 GLU 104 -0.26 ASP 43
ALA 121 0.19 ALA 105 -0.28 ASP 43
ALA 121 0.22 SER 106 -0.25 ASP 43
ALA 121 0.15 ALA 107 -0.23 ASP 43
ALA 121 0.13 ALA 108 -0.23 ASP 43
ALA 121 0.17 GLY 109 -0.22 LEU 17
ALA 121 0.23 LEU 110 -0.25 ASP 43
ALA 121 0.28 VAL 111 -0.25 ASP 43
ALA 121 0.35 TYR 112 -0.24 ASP 43
ALA 121 0.38 GLY 113 -0.25 ASP 43
ALA 121 0.47 LEU 114 -0.29 ASP 43
ALA 121 0.49 THR 115 -0.33 ASP 43
ALA 121 0.65 PRO 117 -0.41 ASP 43
ALA 121 0.59 LEU 118 -0.33 ASP 43
ALA 121 0.69 HIS 119 -0.38 GLY 123
HIS 119 0.52 GLY 120 -0.28 GLY 123
VAL 83 0.96 ALA 121 -0.35 PHE 167
ASP 156 0.39 ARG 122 -0.68 PRO 41
GLU 168 0.49 GLY 123 -0.38 HIS 119
GLU 168 0.32 GLU 124 -0.22 GLU 62
ALA 121 0.25 LEU 125 -0.38 ASP 43
ALA 121 0.27 GLY 126 -0.32 ASP 43
ALA 121 0.36 ALA 127 -0.33 ASP 43
ALA 121 0.35 LEU 128 -0.24 ASP 43
ALA 121 0.34 SER 129 -0.27 ASP 43
ALA 121 0.32 LEU 130 -0.22 ASP 43
ALA 121 0.29 SER 131 -0.22 ASP 43
ALA 121 0.30 VAL 132 -0.19 ASP 43
ALA 121 0.26 GLU 133 -0.21 ALA 21
ALA 121 0.28 ALA 134 -0.20 ALA 21
ALA 121 0.27 GLU 135 -0.20 ALA 21
ALA 121 0.32 ASN 136 -0.19 ASP 43
ALA 121 0.38 ARG 137 -0.20 ASP 43
ALA 121 0.42 ALA 138 -0.18 ASP 43
ALA 121 0.37 GLU 139 -0.17 ASP 43
ALA 121 0.39 ALA 140 -0.19 ASP 43
ALA 121 0.47 ASN 141 -0.20 ASP 43
ALA 121 0.45 ARG 142 -0.17 ASP 43
ALA 121 0.40 PHE 143 -0.17 ASP 43
ALA 121 0.52 GLU 145 -0.21 ASP 43
ALA 121 0.44 SER 146 -0.19 ASP 43
ALA 121 0.43 VAL 147 -0.18 ASP 43
ALA 121 0.54 LEU 148 -0.21 ASP 43
ALA 121 0.57 PRO 149 -0.18 ASP 43
ALA 121 0.46 THR 150 -0.15 ASP 43
ALA 121 0.48 LEU 151 -0.19 ASP 43
ALA 121 0.64 TRP 152 -0.21 ASP 43
ALA 121 0.40 LEU 154 -0.21 GLY 6
ALA 121 0.48 LYS 155 -0.18 ASP 43
ALA 121 0.54 ASP 156 -0.16 ASP 43
ARG 122 0.30 TYR 157 -0.12 ASP 156
ARG 122 0.20 ALA 158 -0.10 ALA 58
ARG 122 0.22 LEU 159 -0.13 GLY 123
ARG 122 0.36 GLN 160 -0.16 ALA 58
LYS 42 0.29 SER 161 -0.18 ALA 58
LYS 42 0.31 GLY 162 -0.24 ALA 58
LYS 42 0.44 ALA 163 -0.26 ALA 58
LYS 42 0.50 GLY 164 -0.32 ALA 121
LYS 42 0.48 LEU 165 -0.33 ALA 58
LYS 42 0.53 ALA 166 -0.42 ALA 58
LYS 42 0.77 PHE 167 -0.39 ALA 58
LYS 42 0.75 GLU 168 -0.41 ALA 58

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

elNémo is maintained by Yves-Henri Sanejouand.
It was developed by Karsten Suhre.
Between 2003 and 2014, it was hosted by IGS (Marseille).
Between 2015 and 2025, it was hosted by US2B (Nantes).
Last modification: december 26th, 2025.