Influence of Random Magnetic Field on Photospheric Surface Waves

Details Influence of Random Magnetic Field on Photospheric Surface Waves Influence of Random Magnetic Field on Photospheric Surface Waves

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.547...69e&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

1

Scientific paper

The discrepancies between theoretically predicted and observed frequencies of solar global oscillations (e.g. pand f-modes) have attracted major attention in the past two decades. In the following we wish to explore whether the solar atmosphere may account for the apparent frequency paradox. Magnetic flux is continuously emerging at photospheric levels and expanding into the solar atmosphere. We investigate the possible effects of an atmospheric random magnetic field on the solar fundamental mode (f-mode).

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