CNRS Nantes University US2B US2B
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Should you encounter any unexpected behaviour,
please let us know.
elNémo has been hacked on november 27th.
It has been moved away and runs again.
**Still some additional cleaning from time to time**
Sorry for the inconvenience.


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CA distance fluctuations for 2602140530321848136

---  normal mode 21  ---

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
PRO 36 0.85 SER 33 -0.55 ILE 50
PRO 36 1.02 PRO 34 -0.37 GLN 38
MET 44 0.32 LEU 35 -0.71 GLU 51
PRO 34 1.02 PRO 36 -0.11 ASP 42
MET 40 0.49 SER 37 -1.00 ASP 41
MET 40 0.38 GLN 38 -0.96 ILE 50
MET 44 0.35 ALA 39 -1.40 GLU 51
SER 33 0.69 MET 40 -0.40 GLU 51
SER 33 0.59 ASP 41 -1.00 SER 37
GLN 52 0.30 ASP 42 -0.28 SER 37
PRO 36 0.38 LEU 43 -0.43 ASP 48
PRO 36 0.52 MET 44 -0.24 ASP 48
PRO 36 0.22 LEU 45 -1.07 ALA 39
ASP 42 0.23 SER 46 -1.23 ILE 50
ASP 42 0.16 PRO 47 -1.27 ALA 39
PHE 54 0.41 ASP 48 -1.15 ALA 39
PHE 54 1.36 ASP 49 -0.95 ALA 39
PHE 54 0.68 ILE 50 -1.23 SER 46
THR 55 1.39 GLU 51 -1.40 ALA 39
ASP 49 0.87 GLN 52 -1.32 ALA 39
ASP 49 1.03 TRP 53 -1.18 SER 46
ASP 49 1.36 PHE 54 -1.23 ALA 39
GLU 51 1.39 THR 55 -1.20 ALA 39

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.