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 31  ---

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
ASP 49 0.71 SER 33 -1.35 SER 46
ASP 49 1.29 PRO 34 -1.13 SER 46
ASP 49 1.14 LEU 35 -0.84 SER 46
ASP 49 0.91 PRO 36 -0.91 SER 46
ASP 49 0.96 SER 37 -0.68 SER 46
ASP 49 1.12 GLN 38 -0.82 SER 33
ASP 49 1.01 ALA 39 -0.90 SER 46
ASP 49 0.54 MET 40 -1.20 SER 33
ASP 49 0.95 ASP 41 -0.83 SER 33
ASP 48 0.18 ASP 42 -1.00 SER 33
ASP 48 0.12 LEU 43 -0.48 PRO 47
SER 33 0.41 MET 44 -0.12 ASP 48
GLN 52 0.51 LEU 45 -0.82 PRO 47
GLN 52 0.31 SER 46 -1.35 SER 33
SER 46 0.00 PRO 47 -1.05 SER 33
ILE 50 1.01 ASP 48 -0.12 MET 44
PRO 34 1.29 ASP 49 -0.35 THR 55
ASP 48 1.01 ILE 50 -0.35 PRO 47
ASP 41 0.58 GLU 51 -0.21 LEU 43
GLN 38 0.72 GLN 52 -0.41 THR 55
ASP 48 0.66 TRP 53 -0.55 SER 33
ASP 48 0.48 PHE 54 -0.53 PRO 47
ASP 48 0.33 THR 55 -0.49 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.