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

NAME

       RNAinverse - manual page for RNAinverse 2.6.4

SYNOPSIS

       RNAinverse [OPTION]...

DESCRIPTION

       RNAinverse 2.6.4

       Find RNA sequences with given secondary structure

       The  program searches for sequences folding into a predefined structure, thereby inverting
       the folding algorithm. Target structures (in bracket notation) and starting sequences  for
       the  search  are read alternately from stdin.  Characters in the start sequence other than
       "AUGC" (or the alphabet specified with -a) will be treated as wild cards and replaced by a
       random  character.  Any  lower  case  characters  in the start sequence will be kept fixed
       during the search. If necessary, the sequence will be  elongated  to  the  length  of  the
       structure.  Thus a string of "N"s as well as a blank line specify a random start sequence.
       For each search the best sequence found and its Hamming distance to the start sequence are
       printed  to stdout. If the the search was unsuccessful, a structure distance to the target
       is appended.  The -Fp and -R options can modify the output format, see commandline options
       below.   The  program  will  continue  to  read  new structures and sequences until a line
       consisting of the single character "@" or an end of file condition is encountered.

       -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

       -v, --verbose
              In conjunction with a negative value supplied to -R, print the last subsequence and
              substructure for each unsuccessful search.

              (default=off)

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

       -F, --function=mp
              Use minimum energy (-Fm), partition function folding (-Fp) or both (-Fmp).

              (default=`m')

              In partition function mode, the probability of the target structure exp(-E(S)/kT)/Q
              is maximized. This probability is written in brackets after the found sequence  and
              Hamming  distance.  In  most  cases you'll want to use the -f option in conjunction
              with -Fp, see below.

       -f, --final=FLOAT
              In combination with -Fp stop search when sequence is found with E(s)-F  is  smaller
              than final, where F=-kT*ln(Q).

       -R, --repeat[=INT]
              Search  repeatedly  for  the  same  structure.   If an argument is supplied to this
              option it must follow the option flag immediately. E.g.: -R5

              (default=`1')

              If repeats is negative search until --repeats exact solutions are found, no  output
              is done for unsuccessful searches. Be aware, that the program will not terminate if
              the target structure can not be found.  If no value is supplied with  this  option,
              the default value is used.

       -a, --alphabet=ALPHABET
              Find sequences using only nucleotides from a given alphabet.

   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.

       --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

       D.H.  Turner, N. Sugimoto, S.M. Freier (1988), "RNA structure prediction", Ann Rev Biophys
       Biophys Chem: 17, pp 167-192

       M. Zuker, P. Stiegler (1981), "Optimal computer  folding  of  large  RNA  sequences  using
       thermodynamic and auxiliary information", Nucl Acid Res: 9, pp 133-148

       J.S.  McCaskill  (1990),  "The  equilibrium  partition  function  and  base  pair  binding
       probabilities for RNA secondary structures", Biopolymers: 29, pp 1105-1119

       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

EXAMPLES

       To  search  5 times for sequences forming a simple hairpin structure interrupted by one GA
       mismatch call

         $ RNAinverse -R 5

       and enter the lines

         (((.(((....))).)))
         NNNgNNNNNNNNNNaNNN

AUTHOR

       Ivo L Hofacker

REPORTING BUGS

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