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 2602140532571859445

---  normal mode 16  ---

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
MET 40 1.39 SER 33 -1.33 PRO 36
MET 40 1.05 PRO 34 -0.61 SER 47
SER 37 0.86 LEU 35 -1.16 SER 33
ALA 39 0.52 PRO 36 -1.33 SER 33
LEU 35 0.86 SER 37 -1.00 ASP 41
MET 40 0.54 GLN 38 -0.94 SER 33
LEU 35 0.56 ALA 39 -0.90 ILE 50
SER 33 1.39 MET 40 -0.47 LEU 43
ASP 49 0.58 ASP 41 -1.00 SER 37
PRO 36 0.31 ASP 42 -0.86 GLN 52
ASP 49 0.44 LEU 43 -0.73 ALA 39
THR 55 1.13 MET 44 -0.52 SER 37
THR 55 0.83 LEU 45 -0.30 ALA 39
LEU 43 0.12 SER 46 -0.31 THR 55
LEU 43 0.40 SER 47 -1.07 PHE 54
PHE 54 0.49 ASP 48 -0.22 ALA 39
GLU 51 0.60 ASP 49 -0.68 ASP 42
PHE 54 0.58 ILE 50 -0.90 ALA 39
MET 44 0.86 GLU 51 -0.70 ALA 39
MET 44 0.97 GLN 52 -0.86 ASP 42
MET 44 0.83 TRP 53 -0.90 SER 47
MET 44 0.94 PHE 54 -1.07 SER 47
MET 44 1.13 THR 55 -0.99 SER 47

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.