The April 8, 2005, Eclipse White-Light Corona View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2006-11-15

AUTHORS

Jay M. Pasachoff, Shelby B. Kimmel, Miloslav Druckmüller, Vojtech Rušin, Metod Saniga

ABSTRACT

The hybrid solar eclipse of April 8, 2005, provided a good opportunity to observe the white-light 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 white-light corona above the west limb ≈260°–270°. We compare this feature with EUV images from SOHO. The feature’s 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. More... »

PAGES

261-270

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s11207-006-0176-4

DOI

http://dx.doi.org/10.1007/s11207-006-0176-4

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1016807156


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