A Bayesian Analysis of MHD Waves in the Lower Atmosphere

Details A Bayesian Analysis of MHD Waves in the Lower Atmosphere A Bayesian Analysis of MHD Waves in the Lower Atmosphere

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..247...48m&link_type=abstract

Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology, Proceedings of the International Astronomical Unio

Astronomy and Astrophysics

Astronomy

Methods: Statistical, Mhd, Sun: Atmosphere, Sun: Photosphere, Sun: Chromosphere, Sun: Transition Region, Sun: Corona, Sun: Oscillations, Waves

Scientific paper

Magneto-hydrodynamic wave modes propagating from the solar photosphere into the corona 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 photospheric p-modes are thought to undergo mode conversion to slow magneto-acoustic waves, and that these slow magnetoacoustic p-modes may be waveguided from the photosphere into the solar corona along the magnetic field. A Bayesian analysis technique is applied to observations which suggests four distinct p-modes may be resolved in the transition region.

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