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dc.contributor.authorMarsal, Santiago
dc.contributor.authorTorta, Joan Miquel
dc.date.accessioned2025-09-10T08:57:29Z
dc.date.available2025-09-10T08:57:29Z
dc.date.issued2019-07-24
dc.identifier.urihttp://hdl.handle.net/20.500.14342/5494
dc.description.abstractWe describe a metric that has been repeatedly applied to assess the performance of models aimed at predicting geomagnetically induced currents from Space Weather events. The used parameterization, based on the well‐known root‐mean‐square error between model and observations, is simple and intuitive. Its use is exemplified, and its advantages and disadvantages are discussed, as well as its relationship with the widely extended correlation coefficient, r. Although the use of r alone is inappropriate for purposes of evaluating the agreement between model and observations, its use is recommended to complement the described performance parameter.ca
dc.format.extent9pca
dc.language.isoengca
dc.relation.ispartofSpace Weather, 17, 941–949ca
dc.rights© American Geophysical Union. Tots els drets reservatsca
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subject.otherGeomagnetically Induced Currentsca
dc.titleQuantifying the Performance of Geomagnetically Induced Current Modelsca
dc.typeinfo:eu-repo/semantics/articleca
dc.rights.accessLevelinfo:eu-repo/semantics/openAccess
dc.embargo.termscapca
dc.identifier.doihttps://doi.org/10.1029/2019SW002208ca
dc.description.versioninfo:eu-repo/semantics/acceptedVersionca


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© American Geophysical Union. Tots els drets reservats
Except where otherwise noted, this item's license is described as http://creativecommons.org/licenses/by-nc-nd/4.0/
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