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 2602140528231840242

---  normal mode 15  ---

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
TRP 53 0.26 SER 33 -1.02 THR 55
TRP 53 0.29 PRO 34 -1.08 THR 55
TRP 53 0.41 LEU 35 -1.06 THR 55
TRP 53 0.50 LEU 36 -1.11 PRO 47
TRP 53 0.57 SER 37 -1.14 PRO 47
TRP 53 0.48 GLN 38 -1.30 PRO 47
TRP 53 0.49 ALA 39 -1.43 PRO 47
TRP 53 0.55 MET 40 -1.67 PRO 47
LEU 45 0.55 ASP 41 -1.54 PRO 47
LEU 45 0.48 ASP 42 -1.53 PRO 47
LEU 45 0.90 LEU 43 -1.33 PRO 47
GLN 52 0.60 MET 44 -1.01 PRO 47
LEU 43 0.90 LEU 45 -0.67 PRO 47
GLN 52 0.59 SER 46 -1.00 GLU 51
GLN 52 0.79 PRO 47 -1.67 MET 40
TRP 53 0.12 ASP 48 -0.42 ALA 39
MET 44 0.26 ASP 49 -0.37 THR 55
GLN 52 0.94 ILE 50 -0.44 THR 55
TRP 53 0.11 GLU 51 -1.00 SER 46
ILE 50 0.94 GLN 52 -0.17 THR 55
SER 37 0.57 TRP 53 -0.14 THR 55
SER 33 0.07 PHE 54 -0.32 LEU 43
SER 33 0.00 THR 55 -1.08 PRO 34

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.