P-mode leakage and Lyman-α intensity

Details P-mode leakage and Lyman-α intensity P-mode leakage and Lyman-α intensity

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..247...74f&link_type=abstract

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

Astronomy and Astrophysics

Astronomy

2

Waves, Sun: Atmosphere, Sun: Photosphere, Sun: Chromosphere, Sun: Oscillations, Sun: Magnetic Fields, Sun: Uv Radiation

Scientific paper

We present an observational test of the hypothesis that leaking p modes heat the solar chromosphere. The amplitude of the leaking p modes in magneto-acoustic portals is determined using MOTH and MDI data. We simulate the propagation of these modes into the chromosphere to determine the height where the wave energy is dissipated by shock waves. A statistical approach is then used to check if this heating process could account for the observed variability of the intensity in the Lyman-α emission.

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