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 26  ---

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
THR 55 0.25 SER 33 -0.15 SER 37
PRO 36 0.18 PRO 34 -0.11 SER 37
ALA 39 0.08 LEU 35 -0.27 SER 37
ALA 39 0.32 PRO 36 -0.11 SER 33
ALA 39 0.34 SER 37 -0.27 LEU 35
PRO 36 0.11 GLN 38 -0.09 SER 33
SER 37 0.34 ALA 39 -0.12 ASP 41
ASP 42 0.18 MET 40 -0.09 SER 33
MET 44 0.13 ASP 41 -0.12 ALA 39
MET 40 0.18 ASP 42 -0.10 ALA 39
PRO 34 0.04 LEU 43 -0.12 LEU 45
ASP 41 0.13 MET 44 -0.10 SER 33
ASP 41 0.08 LEU 45 -0.12 LEU 43
PRO 36 0.05 SER 46 -0.03 SER 33
PRO 34 0.05 PRO 47 -0.09 LEU 45
SER 33 0.05 ASP 48 -0.04 ALA 39
SER 33 0.07 ASP 49 -0.04 ALA 39
SER 33 0.09 ILE 50 -0.06 ALA 39
SER 33 0.13 GLU 51 -0.05 ALA 39
SER 33 0.16 GLN 52 -0.04 ALA 39
SER 33 0.19 TRP 53 -0.05 ALA 39
SER 33 0.22 PHE 54 -0.05 ALA 39
SER 33 0.25 THR 55 -0.04 ALA 39

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.