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 2602140528231840242

---  normal mode 23  ---

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 46 1.21 SER 33 -1.07 THR 55
SER 46 1.24 PRO 34 -0.97 THR 55
SER 46 1.23 LEU 35 -1.01 THR 55
SER 46 1.27 LEU 36 -0.89 THR 55
SER 46 1.33 SER 37 -0.91 THR 55
SER 46 1.66 GLN 38 -0.92 THR 55
SER 46 1.35 ALA 39 -0.77 THR 55
SER 46 1.41 MET 40 -1.11 ASP 42
SER 46 1.64 ASP 41 -0.74 THR 55
SER 46 1.04 ASP 42 -1.11 MET 40
MET 40 1.35 LEU 43 -0.89 TRP 53
PHE 54 0.85 MET 44 -0.66 SER 37
SER 33 0.74 LEU 45 -0.32 PRO 47
GLN 38 1.66 SER 46 -0.51 TRP 53
PHE 54 0.69 PRO 47 -1.09 TRP 53
SER 33 0.61 ASP 48 -0.15 TRP 53
SER 33 0.89 ASP 49 -0.25 TRP 53
SER 33 0.75 ILE 50 -0.49 TRP 53
MET 44 0.74 GLU 51 -0.23 TRP 53
PHE 54 0.22 GLN 52 -0.72 SER 37
SER 33 0.19 TRP 53 -1.09 PRO 47
MET 44 0.85 PHE 54 -0.00 THR 55
SER 33 0.00 THR 55 -1.07 SER 33

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.