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 30  ---

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
SER 37 0.45 SER 33 -1.47 LEU 45
SER 37 0.12 PRO 34 -1.58 MET 44
PRO 34 0.00 LEU 35 -0.62 PRO 47
SER 33 0.00 PRO 36 -1.44 THR 55
SER 33 0.45 SER 37 -0.55 PHE 54
ASP 41 0.13 GLN 38 -0.51 GLN 52
PHE 54 0.66 ALA 39 -0.29 PRO 34
GLN 38 0.13 MET 40 -0.74 PRO 34
ALA 39 0.15 ASP 41 -0.80 SER 46
SER 46 0.31 ASP 42 -1.17 SER 33
SER 46 0.57 LEU 43 -1.24 SER 33
SER 46 0.40 MET 44 -1.58 PRO 34
LEU 43 0.47 LEU 45 -1.47 SER 33
ASP 49 0.69 SER 46 -1.25 SER 33
ASP 49 1.33 PRO 47 -1.43 SER 33
MET 44 0.30 ASP 48 -1.30 SER 33
PRO 47 1.33 ASP 49 -1.10 GLN 52
PRO 47 0.75 ILE 50 -1.18 SER 33
ALA 39 0.55 GLU 51 -1.51 TRP 53
THR 55 0.88 GLN 52 -1.14 SER 33
ALA 39 0.52 TRP 53 -1.51 GLU 51
GLN 52 0.86 PHE 54 -1.37 PRO 36
GLN 52 0.88 THR 55 -1.44 PRO 36

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.