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 22  ---

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
GLN 52 0.71 SER 33 -1.52 THR 55
GLN 52 0.70 PRO 34 -1.49 THR 55
GLN 52 0.74 LEU 35 -1.69 THR 55
GLN 52 0.73 PRO 36 -1.61 THR 55
GLN 52 0.67 SER 37 -1.64 THR 55
GLN 52 0.60 GLN 38 -1.51 THR 55
SER 47 0.80 ALA 39 -1.37 THR 55
SER 47 0.92 MET 40 -1.26 THR 55
SER 47 0.72 ASP 41 -1.24 THR 55
SER 47 0.98 ASP 42 -1.02 THR 55
SER 47 0.97 LEU 43 -0.99 THR 55
SER 47 0.38 MET 44 -0.98 THR 55
LEU 43 0.65 LEU 45 -0.86 THR 55
GLN 52 0.14 SER 46 -0.67 THR 55
ASP 42 0.98 SER 47 -0.70 ILE 50
LEU 43 0.10 ASP 48 -0.54 SER 33
GLU 51 0.33 ASP 49 -1.25 GLN 38
PRO 34 0.65 ILE 50 -0.70 SER 47
SER 33 0.63 GLU 51 -0.28 TRP 53
LEU 35 0.74 GLN 52 -0.08 THR 55
SER 33 0.20 TRP 53 -0.40 SER 47
ASP 49 0.23 PHE 54 -0.43 LEU 43
SER 33 0.00 THR 55 -1.69 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.