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CA distance fluctuations for EXAMPLE1

---  normal mode 8  ---

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]

largest increasereflargest decrease
ILE 50 0.18 PRO 1 -0.08 ASN 98
ILE 50 0.21 GLN 2 -0.05 ASN 98
ILE 50 0.22 ILE 3 -0.05 ASN 98
ILE 50 0.24 THR 4 -0.02 LEU 97
ILE 50 0.27 LEU 5 -0.02 LEU 97
ILE 50 0.23 TRP 6 -0.02 LEU 97
GLY 51 0.21 GLN 7 -0.02 GLY 27
ILE 50 0.25 ARG 8 -0.02 GLY 27
ILE 50 0.24 PRO 9 -0.02 LEU 97
ILE 50 0.19 LEU 10 -0.02 LEU 97
ILE 50 0.16 VAL 11 -0.03 ASN 98
ILE 50 0.11 THR 12 -0.04 ASN 98
ILE 50 0.11 ILE 13 -0.03 ASN 98
ILE 50 0.08 LYS 14 -0.03 ASN 98
GLY 49 0.07 ILE 15 -0.02 ASN 98
GLY 49 0.04 GLY 16 -0.02 ASN 98
GLY 49 0.04 GLY 17 -0.03 ASN 98
GLY 49 0.03 GLN 18 -0.02 ASN 98
ILE 50 0.05 LEU 19 -0.03 ASN 98
ILE 50 0.06 LYS 20 -0.02 PRO 79
ILE 50 0.10 GLU 21 -0.01 ASN 98
ILE 50 0.17 ALA 22 -0.01 ASP 29
ILE 50 0.25 LEU 23 -0.01 ALA 28
ILE 50 0.28 LEU 24 -0.01 ASP 25
ILE 50 0.37 ASP 25 -0.02 ARG 8
ILE 50 0.39 THR 26 -0.02 THR 91
ILE 50 0.48 GLY 27 -0.02 ARG 8
ILE 50 0.44 ALA 28 -0.02 ARG 8
ILE 50 0.35 ASP 29 -0.01 ARG 8
ILE 50 0.27 ASP 30 -0.01 VAL 82
ILE 50 0.22 THR 31 -0.01 VAL 82
GLY 49 0.17 VAL 32 -0.01 PRO 81
GLY 49 0.09 LEU 33 -0.01 GLU 34
PHE 99 0.04 GLU 34 -0.03 PRO 79
PHE 99 0.04 GLU 35 -0.05 ILE 50
PHE 99 0.02 MET 36 -0.04 ILE 54
PHE 99 0.02 SER 37 -0.05 ILE 54
GLY 49 0.02 LEU 38 -0.03 ILE 54
GLY 49 0.02 PRO 39 -0.03 ILE 54
GLY 49 0.03 GLY 40 -0.04 LEU 63
GLY 49 0.03 ARG 41 -0.03 ILE 54
GLY 49 0.03 TRP 42 -0.04 ILE 54
GLY 48 0.03 LYS 43 -0.03 ILE 54
PHE 99 0.04 PRO 44 -0.05 GLY 52
PHE 99 0.06 LYS 45 -0.02 GLY 52
PHE 99 0.09 MET 46 -0.03 GLY 52
ASP 29 0.15 ILE 47 -0.05 THR 80
ALA 28 0.27 GLY 48 -0.08 PRO 79
ALA 28 0.39 GLY 49 -0.09 PRO 79
GLY 27 0.48 ILE 50 -0.12 PRO 79
GLY 27 0.36 GLY 51 -0.08 LYS 55
GLY 27 0.27 GLY 52 -0.07 LYS 55
GLY 27 0.19 PHE 53 -0.05 LYS 55
GLY 27 0.14 ILE 54 -0.08 LYS 55
ALA 28 0.09 LYS 55 -0.08 ILE 54
PHE 99 0.06 VAL 56 -0.05 ILE 54
PHE 99 0.04 ARG 57 -0.05 ILE 54
GLY 49 0.07 GLN 58 -0.01 ILE 54
GLY 49 0.07 TYR 59 -0.02 LYS 55
GLY 49 0.09 ASP 60 -0.02 GLY 94
ILE 50 0.09 GLN 61 -0.03 ARG 41
GLY 49 0.09 ILE 62 -0.03 GLY 40
ILE 50 0.10 LEU 63 -0.04 GLY 40
ILE 50 0.11 ILE 64 -0.03 ASN 98
ILE 50 0.12 GLU 65 -0.04 ASN 98
ILE 50 0.15 ILE 66 -0.05 ASN 98
ILE 50 0.14 CYS 67 -0.06 ASN 98
ILE 50 0.12 GLY 68 -0.07 ASN 98
ILE 50 0.14 HIS 69 -0.06 ASN 98
ILE 50 0.12 LYS 70 -0.05 ASN 98
ILE 50 0.14 ALA 71 -0.03 ASN 98
ILE 50 0.13 ILE 72 -0.03 GLY 40
ILE 50 0.14 GLY 73 -0.02 GLY 94
ILE 50 0.13 THR 74 -0.02 ASP 60
GLY 49 0.13 VAL 75 -0.01 PRO 81
GLY 49 0.11 LEU 76 -0.01 PRO 81
GLY 49 0.05 VAL 77 -0.02 ILE 54
PHE 99 0.05 GLY 78 -0.04 ILE 54
PHE 99 0.06 PRO 79 -0.12 ILE 50
PHE 99 0.07 THR 80 -0.07 GLY 48
GLY 51 0.10 PRO 81 -0.07 GLY 48
GLY 51 0.16 VAL 82 -0.01 ASP 30
ILE 50 0.15 ASN 83 -0.01 ASP 30
ILE 50 0.26 ILE 84 -0.01 ASP 30
ILE 50 0.25 ILE 85 -0.01 ASP 60
ILE 50 0.31 GLY 86 -0.01 ARG 8
ILE 50 0.30 ARG 87 -0.01 ASP 60
ILE 50 0.24 ASN 88 -0.02 ASP 60
ILE 50 0.21 LEU 89 -0.02 ASP 60
ILE 50 0.24 LEU 90 -0.02 THR 26
ILE 50 0.23 THR 91 -0.02 ASP 60
ILE 50 0.19 GLN 92 -0.03 GLY 94
ILE 50 0.19 ILE 93 -0.05 ASN 98
ILE 50 0.21 GLY 94 -0.04 ASN 98
ILE 50 0.24 CYS 95 -0.04 ASN 98
ILE 50 0.27 THR 96 -0.04 HIS 69
ILE 50 0.30 LEU 97 -0.04 CYS 67
ILE 50 0.29 ASN 98 -0.08 PRO 1
ILE 50 0.32 PHE 99 -0.05 PRO 1

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).
Last modification: October 18th, 2018.