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author | KatolaZ <katolaz@yahoo.it> | 2015-10-19 16:30:12 +0100 |
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committer | KatolaZ <katolaz@yahoo.it> | 2015-10-19 16:30:12 +0100 |
commit | a86962cbfd0321387c920a04188512d0de2f3036 (patch) | |
tree | b6c0d31342f7af9d605ee83cfffe251554a307d4 /doc/html/mammult_docsu29.html | |
parent | df8386f75b0538075d72d52693836bb8878f505b (diff) |
First commit of MAMMULT documentation
Diffstat (limited to 'doc/html/mammult_docsu29.html')
-rw-r--r-- | doc/html/mammult_docsu29.html | 100 |
1 files changed, 100 insertions, 0 deletions
diff --git a/doc/html/mammult_docsu29.html b/doc/html/mammult_docsu29.html new file mode 100644 index 0000000..973c83d --- /dev/null +++ b/doc/html/mammult_docsu29.html @@ -0,0 +1,100 @@ +<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN" + "http://www.w3.org/TR/html4/loose.dtd"> +<html > +<head><title>1.2.2.0 compute_rho.py</title> +<meta http-equiv="Content-Type" content="text/html; charset=iso-8859-1"> +<meta name="generator" content="TeX4ht (http://www.cse.ohio-state.edu/~gurari/TeX4ht/)"> +<meta name="originator" content="TeX4ht (http://www.cse.ohio-state.edu/~gurari/TeX4ht/)"> +<!-- html,index=2,3,4,5,next --> +<meta name="src" content="mammult_doc.tex"> +<meta name="date" content="2015-10-19 16:26:00"> +<link rel="stylesheet" type="text/css" href="mammult_doc.css"> +</head><body +> + <!--l. 3--><div class="crosslinks"><p class="noindent">[<a +href="mammult_docsu30.html" >next</a>] [<a +href="mammult_docsu28.html" >prev</a>] [<a +href="mammult_docsu28.html#tailmammult_docsu28.html" >prev-tail</a>] [<a +href="#tailmammult_docsu29.html">tail</a>] [<a +href="mammult_docsu27.html#mammult_docsu29.html" >up</a>] </p></div> + <h5 class="subsubsectionHead"><a + id="x33-320001.2.2"></a><span +class="cmtt-10x-x-109">compute</span><span +class="cmtt-10x-x-109">_rho.py</span></h5> +<!--l. 3--><p class="noindent" ><span +class="cmbx-10x-x-109">NAME</span> +<!--l. 3--><p class="indent" > <span +class="cmbx-10x-x-109">compute</span><span +class="cmbx-10x-x-109">_rho.py </span>- compute the Spearman’s rank correlation coefficient <span +class="cmmi-10x-x-109">ρ</span> +between two rankings. +<!--l. 3--><p class="noindent" ><span +class="cmbx-10x-x-109">SYNOPSYS</span> +<!--l. 3--><p class="indent" > <span +class="cmbx-10x-x-109">compute</span><span +class="cmbx-10x-x-109">_rho.py </span><span +class="cmmi-10x-x-109"><</span><span +class="cmitt-10x-x-109">file1</span><span +class="cmmi-10x-x-109">> <</span><span +class="cmitt-10x-x-109">file2</span><span +class="cmmi-10x-x-109">></span> +<!--l. 20--><p class="noindent" ><span +class="cmbx-10x-x-109">DESCRIPTION</span> +<!--l. 20--><p class="indent" > Compute the Spearman’s rank correlation coefficient <span +class="cmmi-10x-x-109">ρ </span>between two rankings +provided in the input files <span +class="cmti-10x-x-109">file1 </span>and <span +class="cmti-10x-x-109">file2</span>. Each input file contains a list of lines, +where the n-th line contains the value of rank of the n-th node. For instance, <span +class="cmti-10x-x-109">file1</span> +and <span +class="cmti-10x-x-109">file2 </span>might contain the ranks of nodes induced by the degree sequences of +two distinct layers of a multiplex. +<!--l. 20--><p class="indent" > However, the program is pretty general and can be used to compute +the Spearman’s rank correlation coefficient between any generic pair of +rankings. +<!--l. 20--><p class="indent" > N.B.: A C implementation of this program, with the same interface is also +available in the executable file <span +class="cmtt-10x-x-109">compute</span><span +class="cmtt-10x-x-109">_rho</span>. +<!--l. 25--><p class="noindent" ><span +class="cmbx-10x-x-109">OUTPUT</span> +<!--l. 25--><p class="indent" > The program prints on <span +class="cmtt-10x-x-109">stdout </span>the value of the Spearman’s rank correlation +coefficient <span +class="cmmi-10x-x-109">ρ </span>between the two rankings provided as input. +<!--l. 32--><p class="noindent" ><span +class="cmbx-10x-x-109">REFERENCE</span> +<!--l. 32--><p class="indent" > V. Nicosia, V. Latora, “Measuring and modeling correlations in multiplex +networks”, <span +class="cmti-10x-x-109">Phys. Rev. E </span><span +class="cmbx-10x-x-109">92</span>, 032805 (2015). +<!--l. 32--><p class="indent" > Link to paper: <a +href="http://journals.aps.org/pre/abstract/10.1103/PhysRevE.92.032805" class="url" ><span +class="cmtt-10x-x-109">http://journals.aps.org/pre/abstract/10.1103/PhysRevE.92.032805</span></a> +<!--l. 32--><p class="indent" > V. Nicosia, G. Bianconi, V. Latora, M. Barthelemy, “Growing multiplex +networks”, <span +class="cmti-10x-x-109">Phys. Rev. Lett. </span><span +class="cmbx-10x-x-109">111</span>, 058701 (2013). +<!--l. 32--><p class="indent" > Link to paper: <a +href="http://prl.aps.org/abstract/PRL/v111/i5/e058701" class="url" ><span +class="cmtt-10x-x-109">http://prl.aps.org/abstract/PRL/v111/i5/e058701</span></a> +<!--l. 32--><p class="indent" > V. Nicosia, G. Bianconi, V. Latora, M. Barthelemy, “Non-linear growth and +condensation in multiplex networks”, <span +class="cmti-10x-x-109">Phys. Rev. E </span><span +class="cmbx-10x-x-109">90</span>, 042807 (2014). +<!--l. 32--><p class="indent" > Link to paper: <a +href="http://journals.aps.org/pre/abstract/10.1103/PhysRevE.90.042807" class="url" ><span +class="cmtt-10x-x-109">http://journals.aps.org/pre/abstract/10.1103/PhysRevE.90.042807</span></a> + + + + <!--l. 3--><div class="crosslinks"><p class="noindent">[<a +href="mammult_docsu30.html" >next</a>] [<a +href="mammult_docsu28.html" >prev</a>] [<a +href="mammult_docsu28.html#tailmammult_docsu28.html" >prev-tail</a>] [<a +href="mammult_docsu29.html" >front</a>] [<a +href="mammult_docsu27.html#mammult_docsu29.html" >up</a>] </p></div> +<!--l. 3--><p class="indent" > <a + id="tailmammult_docsu29.html"></a> +</body></html> |