Observations of solar pores show higher-frequency magnetic oscillations consistent with propagating waves, while lower-frequency ones exhibit phase differences possibly due to opacity contaminating inversions.
International Conference on Applied Physics and Industrial Engineering 2012 Torrence, C
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The Influence of Opacity on Inferred MHD Wave Signatures in the Lower Solar Atmosphere
Observations of solar pores show higher-frequency magnetic oscillations consistent with propagating waves, while lower-frequency ones exhibit phase differences possibly due to opacity contaminating inversions.