Provided by: vienna-rna_2.6.4+dfsg-1build1_amd64 bug

NAME

       RNApaln - manual page for RNApaln 2.6.4

SYNOPSIS

       RNApaln [OPTION]...

DESCRIPTION

       RNApaln 2.6.4

       RNA alignment based on sequence base pairing propensities

       Uses  string-alignment  techniques to perform fast pairwise structural alignments of RNAs.
       Similar to RNApdist secondary structure  is  incorporated  in  an  approximate  manner  by
       computing  base  pair  probabilities,  which  are  then  reduced  to  a vector holding the
       probability that a base is paired upstream, downstream, or  remains  unpaired.  Such  pair
       propsensity  vectors can then be compared using standard alignment algorithms. In contrast
       to RNApdist, RNApaln performs similarity (instead of distance) alignments, considers  both
       sequence  and  structure  information,  and  uses  affine  (rather than linear) gap costs.
       RNApaln can perform semi-local alignments by using free end gaps, a true  local  alignment
       mode is planned.

       The  same  approach has since been used in the StraL program from Gerhard Steeger's group.
       Since StraL has optimized parameters and a multiple alignment mode, it be be currently the
       better option.

       -h, --help
              Print help and exit

       --detailed-help
              Print help, including all details and hidden options, and exit

       --full-help
              Print help, including hidden options, and exit

       -V, --version
              Print version and exit

   I/O Options:
              Command line options for input and output (pre-)processing

       -B, --printAlignment[=filename]
              Print an "alignment" with gaps of the

       profiles
              The  aligned  structures  are written to filename, if specified Otherwise output is
              written to stdout, unless the -Xm option is set in which case  "backtrack.file"  is
              used.

              (default=`stdout')

              The following symbols are used:

       (      )  essentially upstream (downstream) paired bases

       {      }  weakly upstream (downstream) paired bases

       |      strongly paired bases without preference

       ,      weakly paired bases without preference

       .      essentially unpaired bases.

       --noconv
              Do not automatically substitute nucleotide "T" with "U".

              (default=off)

   Algorithms:
              Select additional algorithms which should be included in the calculations.

       -X, --mode=pmfc
              Set the alignment mode to be used.

              The alignment mode is passed as a single character value. The following options are
              available: 'p' - Compare the structures pairwise, that is  first  with  2nd,  third
              with 4th etc. This is the default.

       'm'    - Calculate the distance matrix between all structures. The output is

              formatted as a lower triangle matrix.

              'f' - Compare each structure to the first one.

              'c' - Compare continuously, that is i-th with (i+1)th structure.

       --gapo=open
              Set the gap open penalty

       --gape=ext
              Set the gap extension penalty

       --seqw=w
              Set the weight of sequence (compared to structure) in the scoring function.

       --endgaps
              Use free end-gaps

              (default=off)

   Energy Parameters:
              Energy parameter sets can be adapted or loaded from user-provided input files

       -T, --temp=DOUBLE
              Rescale energy parameters to a temperature of temp C. Default is 37C.

              (default=`37.0')

       -P, --paramFile=paramfile
              Read energy parameters from paramfile, instead of using the default parameter set.

              Different  sets  of  energy  parameters  for  RNA  and  DNA  should  accompany your
              distribution.  See the RNAlib documentation for details on the  file  format.  When
              passing the placeholder file name "DNA", DNA parameters are loaded without the need
              to actually specify any input file.

       -4, --noTetra
              Do not include special tabulated stabilizing energies for tri-, tetra- and hexaloop
              hairpins.

              (default=off)

              Mostly for testing.

       --salt=DOUBLE
              Set salt concentration in molar (M). Default is 1.021M.

   Model Details:
              Tweak  the  energy  model  and  pairing  rules  additionally  using  the  following
              parameters

       -d, --dangles=INT
              How to treat "dangling end" energies for bases adjacent to helices in free ends and
              multi-loops.

              (default=`2')

              With -d1 only unpaired bases can participate in at most one dangling end.  With -d2
              this check is ignored, dangling energies will be added for the bases adjacent to  a
              helix on both sides in any case; this is the default for mfe and partition function
              folding (-p).   The  option  -d0  ignores  dangling  ends  altogether  (mostly  for
              debugging).   With  -d3 mfe folding will allow coaxial stacking of adjacent helices
              in multi-loops. At the moment the implementation will not allow coaxial stacking of
              the two interior pairs in a loop of degree 3 and works only for mfe folding.

              Note  that  with  -d1  and -d3 only the MFE computations will be using this setting
              while partition function uses -d2 setting,  i.e.  dangling  ends  will  be  treated
              differently.

       --noLP Produce structures without lonely pairs (helices of length 1).

              (default=off)

              For  partition  function  folding  this  only  disallows  pairs that can only occur
              isolated. Other pairs may still occasionally occur as helices of length 1.

       --noGU Do not allow GU pairs.

              (default=off)

       --noClosingGU
              Do not allow GU pairs at the end of helices.

              (default=off)

       --nsp=STRING
              Allow other pairs in addition to the usual AU,GC,and GU pairs.

              Its argument is a comma separated list of additionally allowed pairs. If the  first
              character  is  a  "-"  then  AB  will imply that AB and BA are allowed pairs.  e.g.
              RNAfold -nsp -GA  will allow GA  and  AG  pairs.  Nonstandard  pairs  are  given  0
              stacking energy.

       -e, --energyModel=INT
              Set energy model.

              Rarely  used option to fold sequences from the artificial ABCD... alphabet, where A
              pairs B, C-D etc.  Use the energy parameters for GC (-e 1) or AU (-e 2) pairs.

       --helical-rise=FLOAT
              Set the helical rise of the helix in units of Angstrom.

              (default=`2.8')

              Use with caution! This value will be  re-set  automatically  to  3.4  in  case  DNA
              parameters are loaded via -P DNA and no further value is provided.

       --backbone-length=FLOAT
              Set the average backbone length for looped regions in units of Angstrom.

              (default=`6.0')

              Use  with  caution!  This  value  will  be re-set automatically to 6.76 in case DNA
              parameters are loaded via -P DNA and no further value is provided.

REFERENCES

       If you use this program in your work you might want to cite:

       R. Lorenz, S.H. Bernhart, C. Hoener zu Siederdissen, H. Tafer, C. Flamm, P.F. Stadler  and
       I.L. Hofacker (2011), "ViennaRNA Package 2.0", Algorithms for Molecular Biology: 6:26

       I.L.  Hofacker,  W.  Fontana,  P.F. Stadler, S. Bonhoeffer, M. Tacker, P. Schuster (1994),
       "Fast Folding and Comparison of RNA Secondary Structures", Monatshefte f. Chemie: 125,  pp
       167-188

       R.  Lorenz,  I.L.  Hofacker,  P.F.  Stadler  (2016),  "RNA  folding  with  hard  and  soft
       constraints", Algorithms for Molecular Biology 11:1 pp 1-13

       Bonhoeffer S, McCaskill J  S,  Stadler  P  F,  Schuster  P  (1993),  "RNA  multi-structure
       landscapes", Euro Biophys J: 22, pp 13-24

       The energy parameters are taken from:

       D.H.  Mathews,  M.D.  Disney, D. Matthew, J.L. Childs, S.J. Schroeder, J. Susan, M. Zuker,
       D.H. Turner (2004),  "Incorporating  chemical  modification  constraints  into  a  dynamic
       programming  algorithm  for prediction of RNA secondary structure", Proc. Natl. Acad. Sci.
       USA: 101, pp 7287-7292

       D.H Turner, D.H. Mathews (2009),  "NNDB:  The  nearest  neighbor  parameter  database  for
       predicting  stability of nucleic acid secondary structure", Nucleic Acids Research: 38, pp
       280-282

AUTHOR

       Peter F Stadler, Ivo L Hofacker, Sebastian Bonhoeffer

REPORTING BUGS

       If in doubt our program is right,  nature  is  at  fault.   Comments  should  be  sent  to
       rna@tbi.univie.ac.at.