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  • The hybrid solar eclipse of April 8, 2005, provided a good opportunity to observe the whitelight solar corona, even though the eclipse lasted just 30 seconds and could be seen only from ships in the Pacific Ocean. During the eclipse, we detected a unique cloud of particles in the whitelight corona above the west limb 260deg to 270deg. We compare this feature with EUV images from SOHO. The feature density and temperature seem comparable to a coronal condensation, and, like a coronal condensation, it is connected to the emergence of material from the solar surface without a flare. However, the morphology of the feature shows clear differences from a classical coronal condensation.
  • The hybrid solar eclipse of April 8, 2005, provided a good opportunity to observe the whitelight solar corona, even though the eclipse lasted just 30 seconds and could be seen only from ships in the Pacific Ocean. During the eclipse, we detected a unique cloud of particles in the whitelight corona above the west limb 260deg to 270deg. We compare this feature with EUV images from SOHO. The feature density and temperature seem comparable to a coronal condensation, and, like a coronal condensation, it is connected to the emergence of material from the solar surface without a flare. However, the morphology of the feature shows clear differences from a classical coronal condensation. (en)
  • The hybrid solar eclipse of April 8, 2005, provided a good opportunity to observe the whitelight solar corona, even though the eclipse lasted just 30 seconds and could be seen only from ships in the Pacific Ocean. During the eclipse, we detected a unique cloud of particles in the whitelight corona above the west limb 260deg to 270deg. We compare this feature with EUV images from SOHO. The feature density and temperature seem comparable to a coronal condensation, and, like a coronal condensation, it is connected to the emergence of material from the solar surface without a flare. However, the morphology of the feature shows clear differences from a classical coronal condensation. (cs)
Title
  • The 8 April 2005 Eclipse White-Light Corona
  • The 8 April 2005 Eclipse White-Light Corona (en)
  • The 8 April 2005 Eclipse White-Light Corona (cs)
skos:prefLabel
  • The 8 April 2005 Eclipse White-Light Corona
  • The 8 April 2005 Eclipse White-Light Corona (en)
  • The 8 April 2005 Eclipse White-Light Corona (cs)
skos:notation
  • RIV/00216305:26210/06:PU63692!RIV07-MSM-26210___
http://linked.open.../vavai/riv/strany
  • 261-270
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • S
http://linked.open...iv/cisloPeriodika
  • 11
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
  • 510736
http://linked.open...ai/riv/idVysledku
  • RIV/00216305:26210/06:PU63692
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • solar physics, image processing, total solar eclipse (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • NL - Nizozemsko
http://linked.open...ontrolniKodProRIV
  • [29B4BC69FBEE]
http://linked.open...i/riv/nazevZdroje
  • Solar Physics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 238
http://linked.open...iv/tvurceVysledku
  • Druckmüller, Miloslav
  • Pasachoff, Jay
  • Rušin, Vojtěch
  • Saniga, Metod
  • Kimmel, Shelby
issn
  • 0038-0938
number of pages
http://localhost/t...ganizacniJednotka
  • 26210
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