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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F12%3A00388115%21RIV13-GA0-67985815
rdf:type
n13:Vysledek skos:Concept
dcterms:description
I analyze the maps recording the travel-time shifts caused by averaged plasma anomalies under an %22average supergranule,%22 constructed by means of statistical averaging over 5582 individual supergranules with large divergence signals detected in two months of Helioseismic and Magnetic Imager Dopplergrams. By utilizing a three-dimensional validated time-distance inversion code, I measure a peak vertical velocity of 117 2 m s–1 at depths around 1.2 Mm in the center of the supergranule and a root-mean-square vertical velocity of 21 m s–1 over the area of the supergranule. A discrepancy between this measurement and the measured surface vertical velocity (a few m s–1) can be explained by the existence of the large-amplitude vertical flow under the surface of supergranules with large divergence signals, recently suggested by Duvall & Hanasoge. I analyze the maps recording the travel-time shifts caused by averaged plasma anomalies under an %22average supergranule,%22 constructed by means of statistical averaging over 5582 individual supergranules with large divergence signals detected in two months of Helioseismic and Magnetic Imager Dopplergrams. By utilizing a three-dimensional validated time-distance inversion code, I measure a peak vertical velocity of 117 2 m s–1 at depths around 1.2 Mm in the center of the supergranule and a root-mean-square vertical velocity of 21 m s–1 over the area of the supergranule. A discrepancy between this measurement and the measured surface vertical velocity (a few m s–1) can be explained by the existence of the large-amplitude vertical flow under the surface of supergranules with large divergence signals, recently suggested by Duvall & Hanasoge.
dcterms:title
Inversions for Average Supergranular Flows Using Finite-frequency Kernels Inversions for Average Supergranular Flows Using Finite-frequency Kernels
skos:prefLabel
Inversions for Average Supergranular Flows Using Finite-frequency Kernels Inversions for Average Supergranular Flows Using Finite-frequency Kernels
skos:notation
RIV/67985815:_____/12:00388115!RIV13-GA0-67985815
n13:predkladatel
n17:ico%3A67985815
n3:aktivita
n4:P n4:I
n3:aktivity
I, P(GPP209/12/P568), P(IAA300030808)
n3:cisloPeriodika
2
n3:dodaniDat
n14:2013
n3:domaciTvurceVysledku
n9:8215022
n3:druhVysledku
n15:J
n3:duvernostUdaju
n7:S
n3:entitaPredkladatele
n5:predkladatel
n3:idSjednocenehoVysledku
142847
n3:idVysledku
RIV/67985815:_____/12:00388115
n3:jazykVysledku
n12:eng
n3:klicovaSlova
Sun; interior; helioseismology
n3:klicoveSlovo
n8:Sun n8:interior n8:helioseismology
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[C5F464371164]
n3:nazevZdroje
Astrophysical Journal Letters
n3:obor
n18:BN
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
1
n3:projekt
n10:GPP209%2F12%2FP568 n10:IAA300030808
n3:rokUplatneniVysledku
n14:2012
n3:svazekPeriodika
759
n3:tvurceVysledku
Švanda, Michal
n3:wos
000310581600003
s:issn
2041-8205
s:numberOfPages
5
n19:doi
10.1088/2041-8205/759/2/L29