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Statements

Subject Item
n2:RIV%2F00216305%3A26210%2F14%3APU110865%21RIV15-MSM-26210___
rdf:type
skos:Concept n16:Vysledek
dcterms:description
Prominences constitute the most complex magnetic structures in the solar corona. The ubiquitous presence of their seemingly confined dense and cool plasma in an otherwise million-degree environment remains a puzzle. Using a decade of white light total solar eclipse observations, we show how these images reveal an intricate relationship between prominences and coronal structures both in their immediate vicinity, known as coronal cavities, and in the extended corona out to several solar radii. Observations of suspended prominences and twisted helical structures spanning several solar radii are central to these findings. The different manifestations of the prominence-corona interface that emerge from this study underscore the fundamental role played by prominences in defining and controlling the complex expansion and dynamic behavior of the solar magnetic field in the neighborhood of magnetic polarity reversal regions. This study suggests that the unraveling of prominences and the outward expansion of th Prominences constitute the most complex magnetic structures in the solar corona. The ubiquitous presence of their seemingly confined dense and cool plasma in an otherwise million-degree environment remains a puzzle. Using a decade of white light total solar eclipse observations, we show how these images reveal an intricate relationship between prominences and coronal structures both in their immediate vicinity, known as coronal cavities, and in the extended corona out to several solar radii. Observations of suspended prominences and twisted helical structures spanning several solar radii are central to these findings. The different manifestations of the prominence-corona interface that emerge from this study underscore the fundamental role played by prominences in defining and controlling the complex expansion and dynamic behavior of the solar magnetic field in the neighborhood of magnetic polarity reversal regions. This study suggests that the unraveling of prominences and the outward expansion of th
dcterms:title
EXPLORING THE PROMINENCE-CORONA CONNECTION AND ITS EXPANSION INTO THE OUTER CORONA USING TOTAL SOLAR ECLIPSE OBSERVATIONS EXPLORING THE PROMINENCE-CORONA CONNECTION AND ITS EXPANSION INTO THE OUTER CORONA USING TOTAL SOLAR ECLIPSE OBSERVATIONS
skos:prefLabel
EXPLORING THE PROMINENCE-CORONA CONNECTION AND ITS EXPANSION INTO THE OUTER CORONA USING TOTAL SOLAR ECLIPSE OBSERVATIONS EXPLORING THE PROMINENCE-CORONA CONNECTION AND ITS EXPANSION INTO THE OUTER CORONA USING TOTAL SOLAR ECLIPSE OBSERVATIONS
skos:notation
RIV/00216305:26210/14:PU110865!RIV15-MSM-26210___
n4:aktivita
n8:S
n4:aktivity
S
n4:cisloPeriodika
2
n4:dodaniDat
n6:2015
n4:domaciTvurceVysledku
n9:8961905
n4:druhVysledku
n10:J
n4:duvernostUdaju
n17:S
n4:entitaPredkladatele
n7:predkladatel
n4:idSjednocenehoVysledku
16111
n4:idVysledku
RIV/00216305:26210/14:PU110865
n4:jazykVysledku
n13:eng
n4:klicovaSlova
Sun, solar wind, corona, prominences, magnetic fields
n4:klicoveSlovo
n11:corona n11:prominences n11:Sun n11:solar%20wind n11:magnetic%20fields
n4:kodStatuVydavatele
US - Spojené státy americké
n4:kontrolniKodProRIV
[2A45B38F9A3C]
n4:nazevZdroje
ASTROPHYSICAL JOURNAL
n4:obor
n12:BN
n4:pocetDomacichTvurcuVysledku
1
n4:pocetTvurcuVysledku
3
n4:rokUplatneniVysledku
n6:2014
n4:svazekPeriodika
2014 793
n4:tvurceVysledku
Druckmüller, Miloslav Morgan, Huw Habbal, Shadia Rifai
s:issn
0004-637X
s:numberOfPages
10
n14:organizacniJednotka
26210