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authorKatolaZ <katolaz@yahoo.it>2015-10-19 16:30:12 +0100
committerKatolaZ <katolaz@yahoo.it>2015-10-19 16:30:12 +0100
commita86962cbfd0321387c920a04188512d0de2f3036 (patch)
treeb6c0d31342f7af9d605ee83cfffe251554a307d4 /doc/html/mammult_docsu17.html
parentdf8386f75b0538075d72d52693836bb8878f505b (diff)
First commit of MAMMULT documentation
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+<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN"
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+<head><title>1.1.3.0 cartography_from_deg_vectors.py</title>
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+>
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+ <h5 class="subsubsectionHead"><a
+ id="x20-190001.1.3"></a><span
+class="cmtt-10x-x-109">cartography</span><span
+class="cmtt-10x-x-109">_from</span><span
+class="cmtt-10x-x-109">_deg</span><span
+class="cmtt-10x-x-109">_vectors.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">cartography</span><span
+class="cmbx-10x-x-109">_from</span><span
+class="cmbx-10x-x-109">_deg</span><span
+class="cmbx-10x-x-109">_vectors.py </span>- create a multiplex cartography
+diagram.
+<!--l. 3--><p class="noindent" ><span
+class="cmbx-10x-x-109">SYNOPSYS</span>
+<!--l. 3--><p class="indent" > <span
+class="cmbx-10x-x-109">cartography</span><span
+class="cmbx-10x-x-109">_from</span><span
+class="cmbx-10x-x-109">_deg</span><span
+class="cmbx-10x-x-109">_vectors.py </span><span
+class="cmmi-10x-x-109">&#x003C;</span><span
+class="cmitt-10x-x-109">node</span><span
+class="cmitt-10x-x-109">_deg</span><span
+class="cmitt-10x-x-109">_vectors</span><span
+class="cmmi-10x-x-109">&#x003E;</span>
+<!--l. 14--><p class="noindent" ><span
+class="cmbx-10x-x-109">DESCRIPTION</span>
+<!--l. 14--><p class="indent" > Compute and print on output the total degree and the multiplex
+participation coefficient of all the nodes of a multiplex network whose
+list of node degree vectors is provided as input. The input file is in the
+format:
+<!--l. 14--><p class="indent" > &#x00A0; <span
+class="cmti-10x-x-109">IDn</span><span
+class="cmti-10x-x-109">_deg1 IDn</span><span
+class="cmti-10x-x-109">_deg</span><span
+class="cmti-10x-x-109">_2 ... IDn</span><span
+class="cmti-10x-x-109">_degM</span>
+<!--l. 14--><p class="noindent" >where <span
+class="cmti-10x-x-109">IDn</span><span
+class="cmti-10x-x-109">_degX </span>is the degree of node <span
+class="cmmi-10x-x-109">n </span>at layer <span
+class="cmmi-10x-x-109">X</span>. The input file can be
+generated using the script <span
+class="cmtt-10x-x-109">node</span><span
+class="cmtt-10x-x-109">_degree</span><span
+class="cmtt-10x-x-109">_vectors.py</span>.
+<!--l. 30--><p class="noindent" ><span
+class="cmbx-10x-x-109">OUTPUT</span>
+<!--l. 30--><p class="indent" > The program prints on <span
+class="cmtt-10x-x-109">stdout </span>a list of lines in the format:
+<!--l. 30--><p class="indent" > &#x00A0; <span
+class="cmti-10x-x-109">tot</span><span
+class="cmti-10x-x-109">_deg part</span><span
+class="cmti-10x-x-109">_coeff</span>
+<!--l. 30--><p class="noindent" >where <span
+class="cmti-10x-x-109">tot</span><span
+class="cmti-10x-x-109">_deg </span>is the total degree of the node and <span
+class="cmti-10x-x-109">part</span><span
+class="cmti-10x-x-109">_coeff </span>is the corresponding
+participation coefficient.
+<!--l. 30--><p class="noindent" >As usual, node IDs start from zero and proceed sequentially, without gaps,
+so if one of the lines in the input files contains just zeros, the program
+considers the corresponding node as being isolated on all the layers, and both
+its total degree and multiplex participation coefficient are set equal to
+zero.
+<!--l. 32--><p class="noindent" ><span
+class="cmbx-10x-x-109">REFERENCE</span>
+<!--l. 32--><p class="indent" > F. Battiston, V. Nicosia, V. Latora, &#8220;Structural measures for multiplex
+networks&#8221;, <span
+class="cmti-10x-x-109">Phys. Rev. E </span><span
+class="cmbx-10x-x-109">89</span>, 032804 (2014).
+<!--l. 32--><p class="indent" > Link to paper: <a
+href="http://journals.aps.org/pre/abstract/10.1103/PhysRevE.89.032804" class="url" ><span
+class="cmtt-10x-x-109">http://journals.aps.org/pre/abstract/10.1103/PhysRevE.89.032804</span></a>
+
+
+
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