This HTML5 document contains 45 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/
n20http://linked.opendata.cz/resource/domain/vavai/riv/tvurce/
n8http://linked.opendata.cz/resource/domain/vavai/projekt/
n14http://linked.opendata.cz/resource/domain/vavai/subjekt/
n13http://linked.opendata.cz/ontology/domain/vavai/
n7http://linked.opendata.cz/resource/domain/vavai/zamer/
n11http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F67985815%3A_____%2F12%3A00386866%21RIV13-GA0-67985815/
shttp://schema.org/
skoshttp://www.w3.org/2004/02/skos/core#
n3http://linked.opendata.cz/ontology/domain/vavai/riv/
n19http://bibframe.org/vocab/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n9http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n17http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n10http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n5http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n18http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n6http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n4http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F12%3A00386866%21RIV13-GA0-67985815
rdf:type
skos:Concept n13:Vysledek
dcterms:description
We investigate the temperature sensitivity of these AIA bands for prominence observations, in order to infer the temperature content in an effort to explain the emission. Using the CHIANTI atomic database and previously determined prominence differential emission measure distributions, we build synthetic spectra to establish the main emission-line contributors in the AIA bands. We investigate the temperature sensitivity of these AIA bands for prominence observations, in order to infer the temperature content in an effort to explain the emission. Using the CHIANTI atomic database and previously determined prominence differential emission measure distributions, we build synthetic spectra to establish the main emission-line contributors in the AIA bands.
dcterms:title
On the nature of pronimence emission observed by SDO/AIA On the nature of pronimence emission observed by SDO/AIA
skos:prefLabel
On the nature of pronimence emission observed by SDO/AIA On the nature of pronimence emission observed by SDO/AIA
skos:notation
RIV/67985815:_____/12:00386866!RIV13-GA0-67985815
n13:predkladatel
n14:ico%3A67985815
n3:aktivita
n5:P n5:Z
n3:aktivity
P(GAP209/10/1706), P(GAP209/12/1652), Z(AV0Z10030501)
n3:cisloPeriodika
1
n3:dodaniDat
n4:2013
n3:domaciTvurceVysledku
n20:3741451
n3:druhVysledku
n6:J
n3:duvernostUdaju
n17:S
n3:entitaPredkladatele
n11:predkladatel
n3:idSjednocenehoVysledku
156432
n3:idVysledku
RIV/67985815:_____/12:00386866
n3:jazykVysledku
n10:eng
n3:klicovaSlova
Sun; atmosphere; corona
n3:klicoveSlovo
n9:atmosphere n9:corona n9:Sun
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[5E0614204210]
n3:nazevZdroje
Astrophysical Journal
n3:obor
n18:BN
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
4
n3:projekt
n8:GAP209%2F10%2F1706 n8:GAP209%2F12%2F1652
n3:rokUplatneniVysledku
n4:2012
n3:svazekPeriodika
754
n3:tvurceVysledku
Heinzel, Petr Parenti, S. Golub, L. Schmieder, B.
n3:wos
000306111800066
n3:zamer
n7:AV0Z10030501
s:issn
0004-637X
s:numberOfPages
8
n19:doi
10.1088/0004-637X/754/1/66