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 12  ---

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
ILE 50 0.43 SER 33 -0.61 GLN 52
ILE 50 0.43 PRO 34 -0.65 GLN 52
LEU 45 0.61 LEU 35 -0.81 GLN 52
LEU 45 0.76 PRO 36 -0.92 GLN 52
LEU 45 0.82 SER 37 -1.04 GLN 52
LEU 45 0.58 GLN 38 -0.90 GLN 52
LEU 45 0.59 ALA 39 -0.89 GLN 52
TRP 53 0.73 MET 40 -0.96 GLN 52
TRP 53 0.73 ASP 41 -0.88 GLN 52
TRP 53 0.95 ASP 42 -0.75 GLN 52
TRP 53 1.41 LEU 43 -0.97 GLN 52
SER 37 0.47 MET 44 -1.28 THR 55
SER 37 0.82 LEU 45 -0.89 THR 55
MET 40 0.35 SER 46 -0.22 GLN 52
TRP 53 0.50 PRO 47 -0.30 GLN 52
LEU 43 0.30 ASP 48 -1.14 MET 44
THR 55 0.70 ASP 49 -0.93 SER 37
PRO 34 0.43 ILE 50 -0.25 MET 44
SER 33 0.40 GLU 51 -0.21 PHE 54
THR 55 0.26 GLN 52 -1.04 SER 37
LEU 43 1.41 TRP 53 -1.12 MET 44
ASP 49 0.58 PHE 54 -1.04 MET 44
ASP 49 0.70 THR 55 -1.28 MET 44

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.