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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F11%3A00360915%21RIV12-AV0-67985815
rdf:type
skos:Concept n10:Vysledek
dcterms:description
The ALMA (Atacama Large Millimeter/sub-millimeter Array) is the large interferometer that will consist up to 64 high-precision antennas operating in the 31.3 – 950 GHz frequency range. In this range unique observations in cosmology, cold universe, galaxies, stars and their formations, and so on are expected. Among these objectives there is a unique possibility to observe the Sun and to address outstanding issues of solar physics. The ALMA is shortly described and then the new ESO-ALMA European node (ARC) built at Ondřejov Observatory is presented. The new ARC is the only one in Europe oriented to solar physics. The requirements and limitations for ALMA solar observations, as well as some examples of possible solar-oriented ALMA projects, are mentioned. The ALMA (Atacama Large Millimeter/sub-millimeter Array) is the large interferometer that will consist up to 64 high-precision antennas operating in the 31.3 – 950 GHz frequency range. In this range unique observations in cosmology, cold universe, galaxies, stars and their formations, and so on are expected. Among these objectives there is a unique possibility to observe the Sun and to address outstanding issues of solar physics. The ALMA is shortly described and then the new ESO-ALMA European node (ARC) built at Ondřejov Observatory is presented. The new ARC is the only one in Europe oriented to solar physics. The requirements and limitations for ALMA solar observations, as well as some examples of possible solar-oriented ALMA projects, are mentioned.
dcterms:title
ALMA and soar research ALMA and soar research
skos:prefLabel
ALMA and soar research ALMA and soar research
skos:notation
RIV/67985815:_____/11:00360915!RIV12-AV0-67985815
n10:predkladatel
n11:ico%3A67985815
n3:aktivita
n17:P n17:Z
n3:aktivity
P(IAA300030701), Z(AV0Z10030501)
n3:dodaniDat
n13:2012
n3:domaciTvurceVysledku
n12:9659455 n12:5375681
n3:druhVysledku
n9:D
n3:duvernostUdaju
n19:S
n3:entitaPredkladatele
n18:predkladatel
n3:idSjednocenehoVysledku
185241
n3:idVysledku
RIV/67985815:_____/11:00360915
n3:jazykVysledku
n7:eng
n3:klicovaSlova
high angular resolution; interferometers; radio radiation
n3:klicoveSlovo
n20:interferometers n20:high%20angular%20resolution n20:radio%20radiation
n3:kontrolniKodProRIV
[5D3802F2078B]
n3:mistoKonaniAkce
Giardini Naxos
n3:mistoVydani
Cambridge
n3:nazevZdroje
Advances in Plasma Astrophysics
n3:obor
n21:BN
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
2
n3:projekt
n15:IAA300030701
n3:rokUplatneniVysledku
n13:2011
n3:tvurceVysledku
Karlický, Marian Bárta, Miroslav
n3:typAkce
n4:WRD
n3:zahajeniAkce
2010-09-06+02:00
n3:zamer
n16:AV0Z10030501
s:numberOfPages
3
n5:hasPublisher
Cambridge University Press
n22:isbn
9780521197410