Physics
Scientific paper
Oct 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rspsa.413..415e&link_type=abstract
Royal Society (London), Proceedings, Series A - Mathematical and Physical Sciences (ISSN 0080-4630), vol. 413, no. 1845, Oct. 8,
Physics
Gravity Waves, Magnetic Field Configurations, Magnetohydrodynamic Waves, Solar Magnetic Field, Wave Equations, Gravitational Fields, Interplanetary Magnetic Fields, Solar Corona, Solar Planetary Interactions, Wave Propagation
Scientific paper
By using appropriate geometrical configuration and relevant frequency ranges it is shown that hydromagnetic gravity inertial waves propagating both in the helmet streamers and magnetic sectors of the solar corona exhibit critical layers. It is also pointed out that the absorption of propagating waves by the critical-layer mechanism provides a key factor in stabilizing the solar and interplanetary magnetic fields in counter-effect to over-reflection mechanism and critical-layer escalation of evanescent waves.
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