Physics
Scientific paper
Feb 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pdtg.book.....m&link_type=abstract
Propagation and detection of turbulence generated MHD waves in the lower atmosphere. Technical memo., by Mangis, S. J.. Sep. pr
Physics
3
Magnetohydrodynamic Waves, Solar Atmosphere, Wave Propagation, Numerical Integration, Solar Flares, Turbulence, Wave Equations
Scientific paper
Some basic solar concepts are developed and the limiting effects of the terrestrial atmosphere upon solar observations are investigated. Several theoretical aspects of MHD waves and the frequency spectrum of MHD waves generated by the hydrogen convection zone are discussed. The magnitudes of various observable characteristics of these waves are calculated, and there is a brief discussion of how it is hoped that these characteristics can be observed. It is concluded that the visual changes caused by turbulence generated MHD waves are of sufficient magnitude to be observed by orbiting telescopes now being developed, but that more work needs to be done to determine exactly how and where to observe these changes.
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