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Statements

Subject Item
n2:RIV%2F00216305%3A26210%2F14%3APU108553%21RIV15-MSM-26210___
rdf:type
skos:Concept n16:Vysledek
dcterms:description
White light images of the solar corona, taken during total solar eclipses, capture the complex dynamic relationship between the coronal plasma and the magnetic field. This relationship can be recorded on timescales of seconds to minutes, within a few solar radii above the solar surface. Rays, large-scale loops, and streamers, which are the brightest structures in these images, have shaped current models of the coronal magnetic field and solar wind flow. We show in this work how the application of novel image processing techniques to unique high-resolution white light eclipse images reveals the presence of a new class of structures, reminiscent of smoke rings, faint nested expanding loops, expanding bubbles, and twisted helical structures. These features are interpreted as snapshots of the dynamical evolution of instabilities developing at prominence-corona interfaces and propagating outward with the solar wind. White light images of the solar corona, taken during total solar eclipses, capture the complex dynamic relationship between the coronal plasma and the magnetic field. This relationship can be recorded on timescales of seconds to minutes, within a few solar radii above the solar surface. Rays, large-scale loops, and streamers, which are the brightest structures in these images, have shaped current models of the coronal magnetic field and solar wind flow. We show in this work how the application of novel image processing techniques to unique high-resolution white light eclipse images reveals the presence of a new class of structures, reminiscent of smoke rings, faint nested expanding loops, expanding bubbles, and twisted helical structures. These features are interpreted as snapshots of the dynamical evolution of instabilities developing at prominence-corona interfaces and propagating outward with the solar wind.
dcterms:title
Discovery of aNew Class of Coronal Structures in White Light Eclipse Images Discovery of aNew Class of Coronal Structures in White Light Eclipse Images
skos:prefLabel
Discovery of aNew Class of Coronal Structures in White Light Eclipse Images Discovery of aNew Class of Coronal Structures in White Light Eclipse Images
skos:notation
RIV/00216305:26210/14:PU108553!RIV15-MSM-26210___
n3:aktivita
n12:S
n3:aktivity
S
n3:cisloPeriodika
1
n3:dodaniDat
n6:2015
n3:domaciTvurceVysledku
n17:8961905
n3:druhVysledku
n9:J
n3:duvernostUdaju
n8:S
n3:entitaPredkladatele
n10:predkladatel
n3:idSjednocenehoVysledku
11679
n3:idVysledku
RIV/00216305:26210/14:PU108553
n3:jazykVysledku
n15:eng
n3:klicovaSlova
eclipses, instabilities, solar wind, Sun, corona, filaments, prominences
n3:klicoveSlovo
n4:prominences n4:filaments n4:instabilities n4:corona n4:Sun n4:eclipses n4:solar%20wind
n3:kodStatuVydavatele
US - Spojené státy americké
n3:kontrolniKodProRIV
[CE621CA18158]
n3:nazevZdroje
ASTROPHYSICAL JOURNAL
n3:obor
n11:BL
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
3
n3:rokUplatneniVysledku
n6:2014
n3:svazekPeriodika
2014 (785)
n3:tvurceVysledku
Morgan, Huw Habbal, Shadia Rifai Druckmüller, Miloslav
s:issn
0004-637X
s:numberOfPages
9
n14:organizacniJednotka
26210