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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F07%3A00305088%21RIV08-AV0-67985815
rdf:type
skos:Concept n15:Vysledek
dcterms:description
We present a method to study the penumbral fine structure using data obtained by the spectropolarimeter onboard Hinode. For the first time, the penumbral filaments can be considered as resolved in spectropolarimetric measurements. This enables us to use inversion codes with only one-component model atmospheres, and thus assign the obtained stratifications of plasma parameters directly to the penumbral fine structure. This approach is applied to the limb-side part of the penumbra in active region NOAA 10923. The preliminary results show a clear dependence of the plasma parameters on continuum intensity in the inner penumbra, i.e. weaker and horizontal magnetic field along with increased line-of-sight velocity are found in the low layers of the bright filaments. We present a method to study the penumbral fine structure using data obtained by the spectropolarimeter onboard Hinode. For the first time, the penumbral filaments can be considered as resolved in spectropolarimetric measurements. This enables us to use inversion codes with only one-component model atmospheres, and thus assign the obtained stratifications of plasma parameters directly to the penumbral fine structure. This approach is applied to the limb-side part of the penumbra in active region NOAA 10923. The preliminary results show a clear dependence of the plasma parameters on continuum intensity in the inner penumbra, i.e. weaker and horizontal magnetic field along with increased line-of-sight velocity are found in the low layers of the bright filaments. Je uvedena metoda urcena ke studiu jemne struktury penumbry pri pouziti spektropolarimetrickych dat z Hinode. Poprve jsou rozliseny penumbralni filamenty v pripade mereni spektropolarimetrem. To nam umoznuje pouzivat inverzni kod s pouze jednou slozkou atmosfery a diky tomu urcit rozvrstveni parametru plazmy v jednotlivych filamentech. Tento postup je aplikovan na data pozorovana v penumbre v aktivni oblasti NOAA 10930. Predbezne vysledky ukazuji na zrejmou zavislost mezi parametry plazmy a intenzitou kontinua ve vnitrni penumbre; magneticke pole je slabsi a vice horizontalni a pozorovane rychlosti vyssi v nizkych vrstvach atmosfery v jasnych filamentech.
dcterms:title
The Analysis of Penumbral Fine Structure Using an Advanced Inversion Technique Analýza jemné struktury penumbry s použitím pokročilé inverzní techniky The Analysis of Penumbral Fine Structure Using an Advanced Inversion Technique
skos:prefLabel
The Analysis of Penumbral Fine Structure Using an Advanced Inversion Technique Analýza jemné struktury penumbry s použitím pokročilé inverzní techniky The Analysis of Penumbral Fine Structure Using an Advanced Inversion Technique
skos:notation
RIV/67985815:_____/07:00305088!RIV08-AV0-67985815
n3:strany
S601;S606
n3:aktivita
n13:Z
n3:aktivity
Z(AV0Z10030501)
n3:cisloPeriodika
SP3
n3:dodaniDat
n6:2008
n3:domaciTvurceVysledku
n16:6896332
n3:druhVysledku
n9:J
n3:duvernostUdaju
n12:S
n3:entitaPredkladatele
n14:predkladatel
n3:idSjednocenehoVysledku
409508
n3:idVysledku
RIV/67985815:_____/07:00305088
n3:jazykVysledku
n5:eng
n3:klicovaSlova
data analysis; Sun; sunspots
n3:klicoveSlovo
n8:data%20analysis n8:sunspots n8:Sun
n3:kodStatuVydavatele
JP - Japonsko
n3:kontrolniKodProRIV
[1AAE768F2A9B]
n3:nazevZdroje
Publications of the Astronomical Society of Japan
n3:obor
n10:BN
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
11
n3:rokUplatneniVysledku
n6:2007
n3:svazekPeriodika
59
n3:tvurceVysledku
Nagata, S. Katsukawa, Y. Tsuneta, S. Title, A. M. Bellot Rubio, L. Suematsu, Y. Shimizu, T. Ichimoto, K. Jurčák, Jan Lites, B. Tarbell, T. D.
n3:zamer
n17:AV0Z10030501
s:issn
0004-6264
s:numberOfPages
6