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PASACHOFF , J. KIMMEL, S. DRUCKMÜLLER, M. RUŠIN, V. SANIGA, M.
Original Title
The 8 April 2005 Eclipse White-Light Corona
Type
journal article - other
Language
English
Original Abstract
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.
Key words in English
solar physics, image processing, total solar eclipse
Authors
PASACHOFF , J.; KIMMEL, S.; DRUCKMÜLLER, M.; RUŠIN, V.; SANIGA, M.
RIV year
2006
Released
17. 11. 2006
Publisher
Springer Netherlands
Location
Netherlands
ISBN
0038-0938
Periodical
Solar Physics
Year of study
238
Number
11
State
Kingdom of the Netherlands
Pages from
261
Pages to
270
Pages count
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/" }