Numerical Experiments with Magnetoacoustic Waves in the Solar Atmosphere

Details Numerical Experiments with Magnetoacoustic Waves in the Solar Atmosphere Numerical Experiments with Magnetoacoustic Waves in the Solar Atmosphere

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.3.23n&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

With numerical experiments we explore the feasibility of using high frequency waves for probing the magnetic field in the photosphere and the chromosphere of the Sun. We track monochromatic wave trains that propagates through a magnetically structured, realistic solar atmosphere. When entering the magnetically dominated chromosphere, the waves undergo partial mode conversion and get refracted and reflected. We explore the relationship between wave travel times and the topography of the surface of equal Alfven and sound speeds, viz., the magnetic canopy.

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