Challenges in Coronal Moreton waves

Details Challenges in Coronal Moreton waves Challenges in Coronal Moreton waves

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003padeu..13..121b&link_type=abstract

In: Contributions to NATO Advanced Research Workshop Turbulence, Waves, and Instabilities in the Solar Plasma; Hungary, 16-20 Se

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations with the Extreme Ultraviolet Imaging Telescope (EIT) onboard SOHO have revealed the existence of transient coronal waves which propagate across the visible solar disc and are generated by an impulsive event. Using observational quantities (propagation speed, attenuation length) we derive average values for magnetic field intensity and viscosity in the low corona, i.e. we develop global coronal seismology.

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