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  • 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. (en)
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 (en)
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 (en)
skos:notation
  • RIV/00216305:26210/14:PU108553!RIV15-MSM-26210___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • S
http://linked.open...iv/cisloPeriodika
  • 1
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 11679
http://linked.open...ai/riv/idVysledku
  • RIV/00216305:26210/14:PU108553
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • eclipses, instabilities, solar wind, Sun, corona, filaments, prominences (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [CE621CA18158]
http://linked.open...i/riv/nazevZdroje
  • ASTROPHYSICAL JOURNAL
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 2014 (785)
http://linked.open...iv/tvurceVysledku
  • Druckmüller, Miloslav
  • Habbal, Shadia Rifai
  • Morgan, Huw
issn
  • 0004-637X
number of pages
http://localhost/t...ganizacniJednotka
  • 26210
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