Astronomy and Astrophysics – Astronomy
Scientific paper
May 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spd....34.1510m&link_type=abstract
American Astronomical Society, SPD meeting #34, #15.10; Bulletin of the American Astronomical Society, Vol. 35, p.832
Astronomy and Astrophysics
Astronomy
Scientific paper
The 21 April 2002 X-class solar flare exhibited supra-arcade downflows of the type described by McKenzie and Hudson (1999). The flare was observed simultaneously by several observatories, and the downflows were clearly imaged by TRACE and SOHO/SUMER. We present a comparison of the TRACE and SUMER data concerning the supra-arcade downflows, and demonstrate that the dark downflow features are consistent with regions of locally depressed plasma density. Furthermore, the implications of the oscillatory behavior of the supra-arcade spikes for coronal seismology will be considered.
We gratefully acknowledge support from NASA, DARA, CNES, and ESA.
Innes Davina E.
McKenzie David E.
Wang Tower
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