Theoretical Aspects of MHD Coronal Seismology

Details Theoretical Aspects of MHD Coronal Seismology Theoretical Aspects of MHD Coronal Seismology

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.547..407n&link_type=abstract

Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO a

Computer Science

3

Solar Corona, Loop Oscillations, Mhd Waves

Scientific paper

The revolutionary breakthrough in observational detection of propagating and standing quasi-periodic disturbances of coronal plasma parameters, made in the EUV band with SOHO and TRACE mission instruments, toin terms of magnetohydrodynamic (MHD) waves, has given rise to MHD coronal seismology. This review presents the theoretical background of these studies and reflects current trends in the development of the theory.

Affiliated with

Also associated with

No associations

Rating

Theoretical Aspects of MHD Coronal Seismology does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Theoretical Aspects of MHD Coronal Seismology, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical Aspects of MHD Coronal Seismology will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1550485