This HTML5 document contains 73 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
dctermshttp://purl.org/dc/terms/
yago-reshttp://yago-knowledge.org/resource/
dbohttp://dbpedia.org/ontology/
n11http://dbpedia.org/resource/File:
foafhttp://xmlns.com/foaf/0.1/
n5https://global.dbpedia.org/id/
yagohttp://dbpedia.org/class/yago/
dbthttp://dbpedia.org/resource/Template:
rdfshttp://www.w3.org/2000/01/rdf-schema#
freebasehttp://rdf.freebase.com/ns/
n19http://
n13http://commons.wikimedia.org/wiki/Special:FilePath/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
owlhttp://www.w3.org/2002/07/owl#
wikipedia-enhttp://en.wikipedia.org/wiki/
provhttp://www.w3.org/ns/prov#
dbchttp://dbpedia.org/resource/Category:
dbphttp://dbpedia.org/property/
xsdhhttp://www.w3.org/2001/XMLSchema#
goldhttp://purl.org/linguistics/gold/
wikidatahttp://www.wikidata.org/entity/
dbrhttp://dbpedia.org/resource/

Statements

Subject Item
dbr:Neutron_monitor
rdf:type
yago:Work100575741 yago:PsychologicalFeature100023100 yago:ScientificResearch100641820 yago:Activity100407535 dbo:Spacecraft yago:WikicatCosmic-rayExperiments yago:Experiment100639556 yago:Act100030358 yago:YagoPermanentlyLocatedEntity yago:Abstraction100002137 yago:Event100029378 yago:Research100636921 yago:Investigation100633864
rdfs:label
Neutron monitor
rdfs:comment
A neutron monitor is a ground-based detector designed to measure the number of high-energy charged particles striking the Earth's atmosphere from outer space. For historical reasons the incoming particles are called "cosmic rays", but in fact they are particles, predominantly protons and Helium nuclei. Most of the time, a neutron monitor records galactic cosmic rays and their variation with the 11-year sunspot cycle and 22-year magnetic cycle. Occasionally the Sun emits cosmic rays of sufficient energy and intensity to raise radiation levels on Earth's surface to the degree that they are readily detected by neutron monitors. They are termed "ground level enhancements" (GLE).
foaf:depiction
n13:SpaceEnvironmentOverview_From_19830101.jpg n13:ExtremeEvent_19890926-00h_19890931-24h.jpg n13:Oulu_NM.gif
dcterms:subject
dbc:Cosmic-ray_experiments
dbo:wikiPageID
23240438
dbo:wikiPageRevisionID
1056430596
dbo:wikiPageWikiLink
dbr:Hale_cycle dbr:Paraffin_wax dbr:Elastic_collision dbr:Scott_Forbush dbr:Forbush_decrease dbr:Subatomic_particle dbr:Coronal_Mass_Ejection dbr:Billiard_ball n11:ExtremeEvent_19890926-00h_19890931-24h.jpg dbr:Sunspot_cycle dbr:Mars_Science_Laboratory dbr:Protons dbr:Solar_System dbr:Nucleus_(atomic_structure) dbr:Galactic_cosmic_ray dbr:Curiosity_(rover) dbr:Radiation_assessment_detector dbr:Helium dbr:Neutron dbr:Solar_wind dbr:Cosmic_ray dbr:Particle_detector dbr:Proportional_counter dbr:Lead n11:Oulu_NM.gif dbr:Ground_level_enhancement dbr:John_Alexander_Simpson dbr:University_of_Chicago dbc:Cosmic-ray_experiments dbr:Earth's_atmosphere dbr:Helium-3 dbr:International_Geophysical_Year dbr:Sun dbr:Outer_space dbr:Polyethylene n11:SpaceEnvironmentOverview_From_19830101.jpg dbr:Boron-10 dbr:Real-time_Neutron_Monitor_Database dbr:Electron dbr:Nuclear_reaction
dbo:wikiPageExternalLink
n19:nest.nmdb.eu
owl:sameAs
n5:gFmk yago-res:Neutron_monitor freebase:m.0661915 wikidata:Q17152893
dbp:wikiPageUsesTemplate
dbt:Reflist
dbo:thumbnail
n13:SpaceEnvironmentOverview_From_19830101.jpg?width=300
dbo:abstract
A neutron monitor is a ground-based detector designed to measure the number of high-energy charged particles striking the Earth's atmosphere from outer space. For historical reasons the incoming particles are called "cosmic rays", but in fact they are particles, predominantly protons and Helium nuclei. Most of the time, a neutron monitor records galactic cosmic rays and their variation with the 11-year sunspot cycle and 22-year magnetic cycle. Occasionally the Sun emits cosmic rays of sufficient energy and intensity to raise radiation levels on Earth's surface to the degree that they are readily detected by neutron monitors. They are termed "ground level enhancements" (GLE). The neutron monitor was invented by University of Chicago Professor John A. Simpson in 1948. The "18-tube" NM64 monitor, which today is the international standard, is a large instrument weighing about 36 tons.
gold:hypernym
dbr:Detector
prov:wasDerivedFrom
wikipedia-en:Neutron_monitor?oldid=1056430596&ns=0
dbo:wikiPageLength
11944
foaf:isPrimaryTopicOf
wikipedia-en:Neutron_monitor