Propagation Of P-modes Into The Solar Corona

Details Propagation Of P-modes Into The Solar Corona Propagation Of P-modes Into The Solar Corona

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.1801m&link_type=abstract

American Astronomical Society, SPD meeting #37, #18.01; Bulletin of the American Astronomical Society, Vol. 38, p.246

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Magneto-hydrodynamic (MHD) wave modes are observed to propagate from the photosphere into the corona. These have the potential to be exploited as an observational tool in an analogous way to the use of acoustic waves in helio/terrestrial seismology. In regions of strong magnetic field p-modes are thought to undergo mode conversion to slow magneto-acoustic waves. New observations are presented of the propagation of these slow magneto-acoustic p-modes into the solar corona along the loops emerging from active regions. The prospects for new observations with STEREO and Solar-B are also discussed. This work is supported through the NASA post doctoral program.

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