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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F09%3A00335830%21RIV10-AV0-67985815
rdf:type
skos:Concept n16:Vysledek
dcterms:description
In the recent papers, we introduced a method utilised to measure the flow field. In this paper, in combination with helioseismic data, we estimate the depths in the solar convection envelope, where the detected large-scale flow field is well represented by the surface measurements. We show that the large-scale flow detected by our method represents the motion of plasma in layers down to 10 Mm. The supergranules may therefore be treated as the objects carried by the underlying large-scale velocity field. In the recent papers, we introduced a method utilised to measure the flow field. In this paper, in combination with helioseismic data, we estimate the depths in the solar convection envelope, where the detected large-scale flow field is well represented by the surface measurements. We show that the large-scale flow detected by our method represents the motion of plasma in layers down to 10 Mm. The supergranules may therefore be treated as the objects carried by the underlying large-scale velocity field.
dcterms:title
Large-scale horizontal flows in the solar photosphere IV. On the vertical structure of large-scale horizontal flows Large-scale horizontal flows in the solar photosphere IV. On the vertical structure of large-scale horizontal flows
skos:prefLabel
Large-scale horizontal flows in the solar photosphere IV. On the vertical structure of large-scale horizontal flows Large-scale horizontal flows in the solar photosphere IV. On the vertical structure of large-scale horizontal flows
skos:notation
RIV/67985815:_____/09:00335830!RIV10-AV0-67985815
n3:aktivita
n4:P n4:Z
n3:aktivity
P(IAA300030808), Z(AV0Z10030501), Z(MSM0021620860)
n3:cisloPeriodika
4
n3:dodaniDat
n12:2010
n3:domaciTvurceVysledku
n9:5998921 n9:4033558 n9:8215022
n3:druhVysledku
n18:J
n3:duvernostUdaju
n7:S
n3:entitaPredkladatele
n10:predkladatel
n3:idSjednocenehoVysledku
323227
n3:idVysledku
RIV/67985815:_____/09:00335830
n3:jazykVysledku
n14:eng
n3:klicovaSlova
Sun; photospere; interior
n3:klicoveSlovo
n6:interior n6:photospere n6:Sun
n3:kodStatuVydavatele
NL - Nizozemsko
n3:kontrolniKodProRIV
[B787C074F374]
n3:nazevZdroje
New Astronomy
n3:obor
n15:BN
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
5
n3:projekt
n13:IAA300030808
n3:rokUplatneniVysledku
n12:2009
n3:svazekPeriodika
14
n3:tvurceVysledku
Švanda, Michal Sobotka, Michal Kosovichev, A. G. Duvall, T. L. Klvaňa, Miroslav
n3:wos
000263528200011
n3:zamer
n11:AV0Z10030501 n11:MSM0021620860
s:issn
1384-1076
s:numberOfPages
6