<?xml version="1.0"?><rdf:RDF xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:edm="http://www.europeana.eu/schemas/edm/" xmlns:wgs84_pos="http://www.w3.org/2003/01/geo/wgs84_pos" xmlns:foaf="http://xmlns.com/foaf/0.1/" xmlns:rdaGr2="http://rdvocab.info/ElementsGr2" xmlns:oai="http://www.openarchives.org/OAI/2.0/" xmlns:owl="http://www.w3.org/2002/07/owl#" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:ore="http://www.openarchives.org/ore/terms/" xmlns:skos="http://www.w3.org/2004/02/skos/core#" xmlns:dcterms="http://purl.org/dc/terms/"><edm:WebResource rdf:about="http://www.dlib.si/stream/URN:NBN:SI:doc-6REP6DHJ/1df5085ad7eb-b89-fd0ff-18be3c6-5e94a/PDF"><dcterms:extent>1442 KB</dcterms:extent></edm:WebResource><edm:WebResource rdf:about="http://www.dlib.si/stream/URN:NBN:SI:doc-6REP6DHJ/77f1973e-e93d-4078-8d68-4e23e87c620b/TEXT"><dcterms:extent>31 KB</dcterms:extent></edm:WebResource><edm:TimeSpan rdf:about="2014-2024"><edm:begin xml:lang="en">2014</edm:begin><edm:end xml:lang="en">2024</edm:end></edm:TimeSpan><edm:ProvidedCHO rdf:about="URN:NBN:SI:doc-6REP6DHJ"><dcterms:isPartOf rdf:resource="https://www.dlib.si/details/URN:NBN:SI:spr-OE00UKYR" /><dcterms:issued>2016</dcterms:issued><dc:creator>Vogrinčič, Rok</dc:creator><dc:format xml:lang="sl">13 str.</dc:format><dc:format xml:lang="sl">številka:2</dc:format><dc:format xml:lang="sl">letnik:3</dc:format><dc:identifier>ISSN:2385-8567</dc:identifier><dc:identifier>COBISSID_HOST:3005284</dc:identifier><dc:identifier>URN:URN:NBN:SI:doc-6REP6DHJ</dc:identifier><dc:language>sl</dc:language><dc:publisher xml:lang="sl">Založba Fakultete za matematiko in fiziko Univerze v Ljubljani</dc:publisher><dcterms:isPartOf xml:lang="sl">Matrika</dcterms:isPartOf><dc:subject xml:lang="sl">detekcija VLF valov</dc:subject><dc:subject xml:lang="en">Earth ionosphere</dc:subject><dc:subject xml:lang="sl">ionosfera</dc:subject><dc:subject xml:lang="sl">ionosferske motnje</dc:subject><dc:subject xml:lang="sl">radijski valovi</dc:subject><dc:subject xml:lang="sl">SID monitor</dc:subject><dc:subject xml:lang="en">solar flares</dc:subject><dc:subject xml:lang="sl">sončevi izbruhi</dc:subject><dc:subject xml:lang="en">sudden ionospheric disturbances</dc:subject><dc:subject xml:lang="en">VLF radio waves</dc:subject><dc:subject xml:lang="sl">Zemlja</dc:subject><dcterms:temporal rdf:resource="2014-2024" /><dc:title xml:lang="sl">Monitor za spremljanje nenadnih ionosferskih motenj|</dc:title><dc:description xml:lang="sl">A sudden ionospheric disturbance (SID) is an abnormally high ionization density in the D layer of the Earth's ionosphere caused by a Solar flare. When a Solar flare occurs on the Sun a blast of intense ultraviolet and X-ray radiation hits the dayside of the Earth. This high energy radiation is absorbed by atmospheric particles, raising them to excited states and knocking electrons free in the process of photoionization. The low-altitude ionospheric layers (D and E layer) immediately increase in electron density over the entire dayside. The ionospheric disturbance enhances very low frequency (VLF) radio propagation. With an instrument called the SID monitor, located at Astronomical Geophysical Observatory on the Golovec hill in Ljubljana, we can detect Solar flares by monitoring the signal strength of distant VLF transmitters over the course of time. The recorded SIDs indicate whether Solar flares have taken place</dc:description><dc:description xml:lang="sl">Nenadne ionosferske motnje (SID) so izjemno močne gostote ionizacije v D sloju Zemljine ionosfere, ki jih povzročajo izbruhi na Soncu. Ko se izbruh na Soncu zgodi, sunek močnega ultravijoličnega in rentgenskega sevanja zadane dnevno stran Zemlje. Visoko-energijsko sevanje absorbirajo delci v atmosferi, ki preko procesa foto ionizacije postanejo vzbujeni. Najnižjim slojem obsevane ionosfere (D in E sloj) se gostota elektronov nemudoma poveča. Ionosferske motnje ojačajo širjenje valov zelo nizkih frekvenc (VLF). S SID monitorjem, ki se nahaja na astronomskem geofizikalnem observatoriju Golovec v Ljubljani, lahko detektiramo izbruhe na Soncu tako, da spremljamo moč radijskega signala oddaljenega VLF oddajnika, v odvisnosti od časa. Izmerjena motnja (SID) pove, ali je zares prišlo do Sončevega izbruha</dc:description><edm:type>TEXT</edm:type><dc:type xml:lang="sl">znanstveno časopisje</dc:type><dc:type xml:lang="en">journals</dc:type><dc:type rdf:resource="http://www.wikidata.org/entity/Q361785" /></edm:ProvidedCHO><ore:Aggregation rdf:about="http://www.dlib.si/?URN=URN:NBN:SI:doc-6REP6DHJ"><edm:aggregatedCHO rdf:resource="URN:NBN:SI:doc-6REP6DHJ" /><edm:isShownBy rdf:resource="http://www.dlib.si/stream/URN:NBN:SI:doc-6REP6DHJ/1df5085ad7eb-b89-fd0ff-18be3c6-5e94a/PDF" /><edm:rights rdf:resource="http://rightsstatements.org/vocab/InC/1.0/" /><edm:provider>Slovenian National E-content Aggregator</edm:provider><edm:dataProvider xml:lang="en">National and University Library of Slovenia</edm:dataProvider><edm:object rdf:resource="http://www.dlib.si/streamdb/URN:NBN:SI:doc-6REP6DHJ/maxi/edm" /><edm:isShownAt rdf:resource="http://www.dlib.si/details/URN:NBN:SI:doc-6REP6DHJ" /></ore:Aggregation></rdf:RDF>