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Seismology of flaring coronal loops

Objective

Magnetohydrodynamic (MHD) waves and oscillations, observed in astrophysical, laboratory and space plasmas provide us with an excellent tool for the remote diagnostics of the plasmas, which are, in particular, implemented in the techniques of solar coronal seismology, Earth’s magnetospheric magnetoseismology, and MHD spectroscopy of tokamaks. The identification of MHD modes in quasi-periodic pulsations (QPP) of the emission generated by solar and stellar flares opens up interesting perspectives for the study of fine structuring of the solar corona, as well as for the diagnostics of stellar coronae. The aim of the project is to advance our theoretical understanding of MHD modes of flaring plasma structures and the plasma emission modulation by these modes; to develop and implement plasma diagnostic techniques based upon those modes, to analyse QPP of the flare-generated microwave and X-ray emission and to identify the MHD modes associated with them. The detected QPPs will be exploited to do coronal seismology, i.e. by comparing the observations with the models, deducing physical parameters in the solar corona.

Call for proposal

FP7-PEOPLE-2007-2-1-IEF
See other projects for this call

Coordinator

THE UNIVERSITY OF WARWICK
EU contribution
€ 169 008,08
Address
Kirby Corner Road - University House
CV4 8UW Coventry
United Kingdom

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Region
West Midlands (England) West Midlands Coventry
Activity type
Higher or Secondary Education Establishments
Administrative Contact
Kate Hughes (Ms.)
Links
Total cost
No data