Fine Structures in the White-Light Solar Corona at the 2006 Eclipse

Details Fine Structures in the White-Light Solar Corona at the 2006 Eclipse Fine Structures in the White-Light Solar Corona at the 2006 Eclipse

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...665..824p&link_type=abstract

The Astrophysical Journal, Volume 665, Issue 1, pp. 824-829.

Astronomy and Astrophysics

Astronomy

16

Eclipses, Sun: Corona

Scientific paper

Observations of the total solar eclipse of 2006 March 29, as it crossed Africa from southwest to northeast into a Greek island and beyond, allowed correlations with near-simultaneous coronal observations from several spacecraft, including SOHO and TRACE. New methods of compositing images allow the recovery of higher resolution (1"-2") on coronal features than had normally been available in the past, reaching substantially higher resolutions than are currently available from space. We discuss a variety of the new methods and observations, and use them to provide the most detailed portrait possible of the Sun, at least on 2006 March 29.

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