Detail publikace

The 8 April 2005 Eclipse White-Light Corona

PASACHOFF , J. KIMMEL, S. DRUCKMÜLLER, M. RUŠIN, V. SANIGA, M.

Originální název

The 8 April 2005 Eclipse White-Light Corona

Typ

článek v časopise - ostatní, Jost

Jazyk

angličtina

Originální abstrakt

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.

Klíčová slova v angličtině

solar physics, image processing, total solar eclipse

Autoři

PASACHOFF , J.; KIMMEL, S.; DRUCKMÜLLER, M.; RUŠIN, V.; SANIGA, M.

Rok RIV

2006

Vydáno

17. 11. 2006

Nakladatel

Springer Netherlands

Místo

Netherlands

ISSN

0038-0938

Periodikum

Solar Physics

Ročník

238

Číslo

11

Stát

Nizozemsko

Strany od

261

Strany do

270

Strany počet

10

URL

http://www.springerlink.com/content/311t6810p07x1225/

BibTex

@article{BUT43658,
  author="Jay {Pasachoff} and Shelby {Kimmel} and Miloslav {Druckmüller} and Vojtěch {Rušin} and Metod {Saniga}",
  title="The 8 April 2005 Eclipse White-Light Corona",
  journal="Solar Physics",
  year="2006",
  volume="238",
  number="11",
  pages="10",
  issn="0038-0938",
  url="http://www.springerlink.com/content/311t6810p07x1225/"
}