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 20  ---

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 0.77 SER 33 -0.47 ASP 48
ILE 50 0.70 PRO 34 -0.43 GLN 38
ILE 50 0.83 LEU 35 -0.63 GLN 38
ALA 39 0.93 LEU 36 -0.23 SER 46
ILE 50 0.86 SER 37 -0.58 SER 46
MET 40 0.97 GLN 38 -0.63 LEU 35
LEU 36 0.93 ALA 39 -1.03 ASP 41
GLN 38 0.97 MET 40 -0.58 ASP 42
MET 44 0.81 ASP 41 -1.03 ALA 39
PRO 47 0.52 ASP 42 -0.96 ALA 39
PRO 47 0.73 LEU 43 -1.24 SER 46
MET 40 0.88 MET 44 -1.12 SER 46
GLU 51 0.43 LEU 45 -0.73 TRP 53
TRP 53 0.86 SER 46 -1.24 LEU 43
LEU 36 0.76 PRO 47 -0.12 THR 55
PHE 54 0.17 ASP 48 -0.47 SER 33
SER 37 0.28 ASP 49 -0.34 THR 55
SER 37 0.86 ILE 50 -0.30 THR 55
SER 37 0.75 GLU 51 -0.23 THR 55
SER 46 0.48 GLN 52 -0.37 SER 33
SER 46 0.86 TRP 53 -0.73 LEU 45
SER 46 0.76 PHE 54 -0.61 LEU 45
SER 46 0.76 THR 55 -0.54 LEU 45

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.