Detail publikace
The 8 April 2005 Eclipse White-Light Corona
PASACHOFF , J. KIMMEL, S. DRUCKMÜLLER, M. RUŠIN, V. SANIGA, M.
Anglický název
The 8 April 2005 Eclipse White-Light Corona
Typ
Článek recenzovaný mimo WoS a Scopus
Jazyk
en
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.
Vydáno
2006-11-17
Nakladatel
Springer Netherlands
Místo
Netherlands
ISSN
0038-0938
Časopis
SOLAR PHYSICS
Ročník
238
Číslo
11
Strany od–do
261–
Počet stran
10
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/"
}