Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004padeu..14..141e&link_type=abstract
In: Proceedings of the British-Hungarian N+N Workshop for Young Researchers On Computer processing and use of satellite data in
Astronomy and Astrophysics
Astrophysics
Scientific paper
The discrepancies between theoretically predicted and observed frequencies of solar global oscillations (e.g. p- and f-modes) have attracted major attention in the past two decades. In the following we wish to explore further 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).
Erdelyi Robert
Kerekes Andrea
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