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.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Overview paper introducing the Sunrise III balloon-borne solar observatory, its 2024 flight, data volume, and the focus issue containing first scientific results.
citing papers explorer
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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.
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Sunrise III: Instrument, mission, data, and first results
Overview paper introducing the Sunrise III balloon-borne solar observatory, its 2024 flight, data volume, and the focus issue containing first scientific results.