<?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-EAPWHXRD/a0c7e5e6-d709-4c5b-a6f0-2280c80f96d7/PDF"><dcterms:extent>1365 KB</dcterms:extent></edm:WebResource><edm:WebResource rdf:about="http://www.dlib.si/stream/URN:NBN:SI:doc-EAPWHXRD/b3bf6764-b2f7-42b4-af27-6d79d9540985/TEXT"><dcterms:extent>33 KB</dcterms:extent></edm:WebResource><edm:TimeSpan rdf:about="1973-2025"><edm:begin xml:lang="en">1973</edm:begin><edm:end xml:lang="en">2025</edm:end></edm:TimeSpan><edm:ProvidedCHO rdf:about="URN:NBN:SI:doc-EAPWHXRD"><dcterms:isPartOf rdf:resource="https://www.dlib.si/details/URN:NBN:SI:spr-KHWREVIC" /><dcterms:issued>2024</dcterms:issued><dc:creator>Čop, Rudi</dc:creator><dc:format xml:lang="sl">številka:3</dc:format><dc:format xml:lang="sl">letnik:68</dc:format><dc:format xml:lang="sl">str. 361-369</dc:format><dc:identifier>ISSN:0351-0271</dc:identifier><dc:identifier>DOI:10.15292/geodetski-vestnik.2024.03.360-369</dc:identifier><dc:identifier>COBISSID:212264707</dc:identifier><dc:identifier>URN:URN:NBN:SI:doc-EAPWHXRD</dc:identifier><dc:language>sl</dc:language><dc:publisher xml:lang="sl">Zveza geodetov Slovenije</dc:publisher><dcterms:isPartOf xml:lang="sl">Geodetski vestnik</dcterms:isPartOf><dc:subject xml:lang="en">accelerations in the energy density</dc:subject><dc:subject xml:lang="en">energy density in the local magnetic field</dc:subject><dc:subject xml:lang="en">geomagnetic indices</dc:subject><dc:subject xml:lang="sl">geomagnetne nevihte</dc:subject><dc:subject xml:lang="sl">geomagnetni indeksi</dc:subject><dc:subject xml:lang="sl">magnetno polje</dc:subject><dc:subject xml:lang="en">severe geomagnetic storm</dc:subject><dc:subject xml:lang="en">solar cycles</dc:subject><dc:subject xml:lang="sl">Sonce</dc:subject><dc:subject xml:lang="sl">sončevi cikli</dc:subject><dc:subject xml:lang="sl">Zemlja</dc:subject><dcterms:temporal rdf:resource="1973-2025" /><dc:title xml:lang="sl">Spremembe v gostoti energije magnetnega polja Zemlje med geomagnetno nevihto G5 11. maja 2024| Changes in the energy density of the Earth's magnetic field during the G5 geomagnetic storm on May 11, 2024|</dc:title><dc:description xml:lang="sl">Geomagnetic storms are the largest disturbance in the Earth's magnetic field. On May 11, 2024, a geomagnetic storm occurred at the peak of the 25th solar cycle, reaching the highest level (G5) on the planetary scale. On that day, a geomagnetic storm was also measured at the PIA geomagnetic observatory (Piran, Slovenia), reaching the maximum possible value of the geomagnetic index K = 9. Such strong geomagnetic storms occur on average every 40 to 60 years. A geomagnetic storm with an index of K = 9 represents an important reference for all disturbances in the local magnetic field from different sources and different intensities. Therefore, an analysis of accelerations in the energy density of the local magnetic field during the first 150 days in 2024 was made. The identified effects of geomagnetic storms with different K indices will serve to better analyse disturbances in the local magnetic field that have occurred in the past years and will happen in the future</dc:description><dc:description xml:lang="sl">Geomagnetne nevihte so največja motnja v Zemljinem magnetnem polju. Dne 11. maja 2024, v maksimumu 25. sončevega cikla, je nastala geomagnetna nevihta, ki je na planetarni ravni dosegla najvišjo stopnjo G5. Tudi na geomagnetnem observatoriju PIA (Piran, Slovenia) je bila tisti dan izmerjena geomagnetna nevihta, ki je dosegla največjo možno vrednost geomagnetnega indeksa K = 9. Tako močne geomagnetne nevihte se v povprečju pojavljajo na vsakih štirideset do šestdeset let. Geomagnetna nevihta z indeksom K = 9 je pomembna referenca za vse motnje v lokalnem magnetnem polju iz različnih izvorov in različnih jakosti. Zato je bila narejena analiza pospeškov v gostoti energije lokalnega magnetnega polja v prvih 150 dneh v letu 2024. Ugotovljeni učinki geomagnetnih neviht z različnimi indeksi K bodo podlaga za boljšo analizo motenj v lokalnem magnetnem polju, ki so se zgodile v preteklih letih ali se bodo zgodile v prihodnje</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-EAPWHXRD"><edm:aggregatedCHO rdf:resource="URN:NBN:SI:doc-EAPWHXRD" /><edm:isShownBy rdf:resource="http://www.dlib.si/stream/URN:NBN:SI:doc-EAPWHXRD/a0c7e5e6-d709-4c5b-a6f0-2280c80f96d7/PDF" /><edm:rights rdf:resource="http://creativecommons.org/licenses/by-nc/4.0/" /><edm:provider>Slovenian National E-content Aggregator</edm:provider><edm:intermediateProvider xml:lang="en">National and University Library of Slovenia</edm:intermediateProvider><edm:dataProvider xml:lang="sl">Zveza geodetov Slovenije</edm:dataProvider><edm:object rdf:resource="http://www.dlib.si/streamdb/URN:NBN:SI:doc-EAPWHXRD/maxi/edm" /><edm:isShownAt rdf:resource="http://www.dlib.si/details/URN:NBN:SI:doc-EAPWHXRD" /></ore:Aggregation></rdf:RDF>