Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004padeu..14..153b&link_type=abstract
In: Proceedings of the British-Hungarian N+N Workshop for Young Researchers On Computer processing and use of satellite data in
Astronomy and Astrophysics
Astrophysics
Scientific paper
Observations with the Extreme Ultraviolet Imaging Telescope (EIT) onboard SOHO have revealed the existence of transient coronal wave-like phenomena which are generated by an impulsive event and propagate across the visible solar disk for very long distances. Since these waves are able to carry information about the plasma in which they propagate, they are a perfect tool for coronal plasma diagnostics. We propose to study these waves to obtain information about the average values of the magnetic field and mean transport coefficients in the quiet Sun. The present contribution answers some of the 'hottest' questions related to the nature and proprieties of EIT waves.
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