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 2602140525071824790

---  normal mode 11  ---

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
SER 37 0.12 SER 33 -0.53 ASP 41
MET 40 0.17 PRO 34 -0.48 ASP 41
PRO 34 0.00 LEU 35 -1.31 ASP 48
THR 55 0.73 PRO 36 -0.00 LEU 35
PHE 54 1.27 SER 37 -0.04 LEU 35
PHE 54 0.90 GLN 38 -0.14 LEU 35
PHE 54 0.38 ALA 39 -0.29 LEU 35
SER 37 0.35 MET 40 -1.75 LEU 43
LEU 43 0.50 ASP 41 -0.63 LEU 35
SER 37 0.57 ASP 42 -0.75 MET 40
SER 37 0.52 LEU 43 -1.75 MET 40
SER 37 0.45 MET 44 -1.07 MET 40
SER 37 0.61 LEU 45 -1.03 LEU 35
SER 37 0.64 SER 46 -1.25 LEU 35
SER 37 0.79 PRO 47 -1.29 LEU 35
SER 37 0.83 ASP 48 -1.31 LEU 35
SER 37 0.82 ASP 49 -1.11 LEU 35
SER 37 0.95 ILE 50 -1.02 LEU 35
SER 37 1.07 GLU 51 -1.10 LEU 35
SER 37 1.03 GLN 52 -1.02 LEU 35
SER 37 1.10 TRP 53 -0.85 LEU 35
SER 37 1.27 PHE 54 -0.87 LEU 35
SER 37 1.22 THR 55 -0.93 LEU 35

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.