The April 8, 2005, Eclipse White-Light Corona

Details The April 8, 2005, Eclipse White-Light Corona The April 8, 2005, Eclipse White-Light Corona

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006soph..238..261p&link_type=abstract

Solar Physics, Volume 238, Issue 2, pp.261-270

Physics

10

Scientific paper

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.

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