<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2015-09-17T11:45:00Z" status="active" updated="2024-12-27T08:31:05Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vg="http://www.ivoa.net/xml/VORegistry/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/VORegistry/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VORegistry.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:DataService"><title>NMDB: Real-time Database for High Resolution Neutron Monitor
Measurements</title><shortName>nmdb web</shortName><identifier>ivo://org.gavo.dc/gvo/data/nmdb/run</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Steigies, C.</name></creator><creator><name>Kudela, K.</name></creator><creator><name>Usoskin, I.</name></creator><creator><name>Flückiger, E.O.</name></creator><creator><name>Eroshenko, E.</name></creator><creator><name>Mavromichalaki, H.</name></creator><creator><name>Klein, K.-L.</name></creator><creator><name>Chilingaryan, A.</name></creator><creator><name>Kryakunova, O.</name></creator><creator><name>Dorman, L.</name></creator><creator><name>Medina, J.</name></creator><contact><name>NMDB Team</name><email>questions@nmdb.eu</email></contact></curation><content><subject>cosmic-rays</subject><subject>forbush-effect</subject><subject>solar-particle-emission</subject><subject>solar-neutrons</subject><description> NMDB serves the data of roughly 50 stations across the globe
measuring ground-based cosmic ray intensities at minute cadence.
Cosmic rays are detected for primary particles of energies up to 15
GeV depending on station magnetic latitude.</description><source format="bibcode">2010ASPC..424...75M</source><referenceURL>http://dc.g-vo.org/gvo/data/nmdb/run/info</referenceURL><contentLevel>Research</contentLevel></content><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">http://nest.nmdb.eu</accessURL></interface></capability><capability standardID="ivo://ivoa.net/std/VOSI#capabilities"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="full">http://dc.g-vo.org/gvo/data/nmdb/run/capabilities</accessURL><mirrorURL>https://dc.g-vo.org/gvo/data/nmdb/run/capabilities</mirrorURL></interface></capability></ri:Resource>