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 2602140530321848136

---  normal mode 19  ---

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
MET 40 1.05 SER 33 -0.55 MET 44
THR 55 0.59 PRO 34 -0.38 MET 44
SER 33 0.19 LEU 35 -0.44 MET 44
THR 55 0.72 PRO 36 -0.21 LEU 43
SER 33 0.38 SER 37 -0.87 MET 40
SER 33 0.21 GLN 38 -0.93 MET 44
SER 33 0.38 ALA 39 -0.78 PHE 54
SER 33 1.05 MET 40 -0.87 SER 37
ASP 48 0.81 ASP 41 -0.87 MET 44
PRO 36 0.15 ASP 42 -0.46 GLN 52
ASP 48 0.59 LEU 43 -0.76 GLN 38
ASP 48 0.40 MET 44 -0.93 GLN 38
ILE 50 0.38 LEU 45 -0.33 SER 37
ASP 49 0.91 SER 46 -0.44 SER 37
ILE 50 0.91 PRO 47 -0.57 SER 37
ASP 41 0.81 ASP 48 -1.09 GLU 51
SER 46 0.91 ASP 49 -0.44 ASP 42
PRO 47 0.91 ILE 50 -0.60 ALA 39
PRO 36 0.50 GLU 51 -1.09 ASP 48
SER 46 0.71 GLN 52 -0.57 ALA 39
SER 46 0.76 TRP 53 -0.61 ALA 39
PRO 36 0.65 PHE 54 -0.78 ALA 39
PRO 36 0.72 THR 55 -0.71 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.