Computer Science – Sound
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79..327b&link_type=abstract
Solar Physics, vol. 79, Aug. 1982, p. 327-331.
Computer Science
Sound
1
Atmospheric Effects, Radiation Pressure, Solar Atmosphere, Solar Corona, Sound Waves, Hydrostatic Pressure, Magnetohydrodynamic Waves, Plasma Heating, Pressure Effects
Scientific paper
While light pressure can be neglected in the hydrostatic balance of the solar atmosphere, radiation pressure due to acoustic waves and Alfven waves is higher and must be taken into account. Acoustic radiation pressure in the solar atmosphere is generated by absorption of sound energy, reflection of sound energy, and change of sound velocity, with pressure caused by absorption dominating within the solar corona. Radiation pressure caused by reflection, and the wave velocity change, probably produce a pressure inversion in the transition zone between chromosphere and corona. In addition, spicule phenomena are due to nonstationary radiation pressure.
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