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Global coronal seismology View all abstracts by submitter

Istvan Ballai   Submitted: 2007-03-20 11:59

Following the observation and analysis of large-scale coronal wave-like disturbances, we discuss the theoretical progress made in the field of global coronal seismology. Using simple mathematical techniques we determine average values for magnetic field together with a magnetic map of the quiet Sun. The interaction between global coronal waves and coronal loops allows us to study loop oscillations in a much wider context, i.e. we connect global and local coronal oscillations.

Authors: Istvan Ballai
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Publication Status: Solar Physics (in press)
Last Modified: 2007-04-12 02:57
Go to main E-Print page  Keynote Address: Outstanding Problems in Solar Physics  Coronal Magnetic Connectivity and EUV Dimmings  Edit Entry  Download Preprint  Delete Entry 

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