On the absence of critical levels in the solar atmosphere

Details On the absence of critical levels in the solar atmosphere On the absence of critical levels in the solar atmosphere

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...92..133s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 92, May 1984, p. 133-144.

Physics

24

Solar Atmosphere, Solar Magnetic Field, Solar Oscillations, Solar Physics, Atmospheric Stratification, Differential Equations, Vibration Mode, Wave Equations

Scientific paper

The authors consider the propagation of linear oscillations in a stratified atmosphere permeated by an oblique but nearly horizontal uniform magnetic field. The results do not show any of the strong characteristics associated with critical level singularities in the exactly horizontal field case. This suggests that critical levels may be of more mathematical interest than physical relevance in the solar atmosphere where the planar horizontal field approximation is seldom adequate.

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