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RNAPDIST(1) User Commands RNAPDIST(1) NAME RNApdist - manual page for RNApdist 2.7.2 SYNOPSIS RNApdist [OPTION]... DESCRIPTION RNApdist 2.7.2 Calculate distances between thermodynamic RNA secondary structures ensem- bles This program reads RNA sequences from stdin and calculates structure dis- tances between the thermodynamic ensembles of their secondary structures. To do this the partition function and matrix of base pairing probabilities is computed for each sequence. The probability matrix is then condensed into a vector holding for each base the probabilities of being unpaired, paired upstream, or paired downstream, respectively. These profiles are compared by a standard alignment algorithm. The base pair probabilities are also saved as postscript "dot plots" (as in RNAfold) in the files "name_dp.ps", where name is the name of the se- quence, or a number if unnamed. -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 Be verbose. (default=off) Lower the log level setting such that even INFO messages are passed through. I/O Options: Command line options for input and output (pre-)processing --noconv Do not automatically substitute nucleotide "T" with "U". (default=off) --log-level=level Set log level threshold. (default=`2') By default, any log messages are filtered such that only warnings (level 2) or errors (level 3) are printed. This setting allows for specifying the log level threshold, where higher values result in fewer information. Log-level 5 turns off all messages, even errors and other critical information. --log-file[=filename] Print log messages to a file instead of stderr. (de- fault=`RNApdist.log') --log-time Include time stamp in log messages. (default=off) --log-call Include file and line of log calling function. (default=off) Algorithms: Select additional algorithms which should be included in the calcu- lations. -X, --compare=p|m|f|c Specify the comparison directive. (default=`p') Possible arguments for this option are: -Xp compare the structures pairwise (p), i.e. first with 2nd, third with 4th etc. -Xm calcu- late the distance matrix between all structures. The output is for- matted as a lower triangle matrix. -Xf compare each structure to the first one. -Xc compare continuously, that is i-th with (i+1)th structure. -B, --backtrack[=<filename>] Print an "alignment" with gaps of the profiles. The aligned struc- tures are written to <filename>, if specified. (default=`none') Within the profile output, the following symbols will be used: () essentially upstream (downstream) paired bases {} weakly upstream (downstream) paired bases | strongly paired bases without preference , weakly paired bases without preference . essentially unpaired bases. If <filename> is not specified, the output is written to stdout, un- less the "-Xm" option is set in which case "backtrack.file" is used. 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 para- meters 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 fol- lowing parameters -d, --dangles=INT set energy model for treatment of dangling bases. (possible values="0", "2" default=`2') --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 he- lices 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. --energyModel=INT Set energy model. Rarely used option to fold sequences from the artificial ABCD... al- phabet, where A pairs B, C-D etc. Use the energy parameters for GC (--energyModel 1) or AU (--energyModel 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 S. Bonhoeffer, J.S. McCaskill, P.F. Stadler, P. Schuster (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. Su- san, M. Zuker, D.H. Turner (2004), "Incorporating chemical modification constraints into a dynamic programming algorithm for prediction of RNA sec- ondary 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", Nu- cleic 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. RNApdist 2.7.2 December 2025 RNAPDIST(1)
NAME | SYNOPSIS | DESCRIPTION | REFERENCES | AUTHOR | REPORTING BUGS
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