Mercurial > repos > ecology > pampa_communitymetrics
view CalculateCommunityMetrics.xml @ 1:e2b0eec4e788 draft
"planemo upload for repository https://github.com/ColineRoyaux/PAMPA-Galaxy commit a7eec629a3f306456d24732b1f365863d1575902"
author | ecology |
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date | Wed, 22 Jul 2020 11:43:46 -0400 |
parents | ddd5b2e74b8b |
children | eda3985e8efb |
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<tool id="pampa_communitymetrics" name="Calculate community metrics" version="@VERSION@"> <description>calculate community metrics from abundance data</description> <macros> <import>pampa_macros.xml</import> </macros> <expand macro="Pampa_requirements"/> <command detect_errors="exit_code"><![CDATA[ Rscript '$__tool_directory__/FunctExeCalcCommIndexesGalaxy.r' '$input' '$indexes' '$__tool_directory__/FunctPAMPAGalaxy.r' '$output_community' ]]> </command> <inputs> <expand macro="pampa_input_calculate"/> <param name="indexes" type="select" label="Choose the community metrics you want to compute" help="Presence/absence, Species richness, Simpson and Shannon index are systematically computed." multiple="true"> <option selected="true" value="all">All</option> <option value="simpson.l">1-Simpson</option> <option value="pielou">Pielou</option> <option value="hill">Hill</option> </param> </inputs> <outputs> <data name="output_community" from_work_dir="TabCommunityIndexes.tabular" format="tabular"/> </outputs> <tests> <test> <param name="input" value="ObservationsSansszcl_cropped.tabular"/> <param name="indexes" value="all"/> <output name="output_community" value="Community_metrics_cropped.tabular"/> </test> </tests> <edam_topics> <edam_topic>topic_0610</edam_topic> </edam_topics> <help><![CDATA[ =============================================== Calculate community metrics from abundance data =============================================== **What it does** This tool from PAMPA toolsuite computes community metrics from abundance data: - Specific richness - Shannon index - Simpson index - Pielou index - Hill index - Relative richness | **Input description** A tabular file with observation data. Must at least contain three columns 'observation.unit' which associate year and location or 'year' and 'location', 'species.code' with species ID and 'number' for abundance. +------------------+--------------+------------+ | observation.unit | species.code | number | +==================+==============+============+ | site_yearID | speciesID | 4 | +------------------+--------------+------------+ | ... | ... | ... | +------------------+--------------+------------+ OR +------+----------+--------------+------------+ | year | location | species.code | number | +======+==========+==============+============+ | 2000 |locationID| speciesID | 4 | +------+----------+--------------+------------+ | ... | ... | ... | ... | +------+----------+--------------+------------+ The data frame may also contain: - 'size.class' field with 'G' representing big individuals in given species, 'M' middle-sized individuals and 'P' small individuals - 'rotation' field for STAVIRO data | **Output** A tabular file with every metrics selected computed per observation unit | **Source** Derived from PAMPA scripts (https://wwz.ifremer.fr/pampa/Meth.-Outils/Outils) written by Yves Reecht. ]]></help> <expand macro="pampa_bibref" /> </tool>