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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Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
SKA+VLBI will enable routine mas-scale imaging of nearby extragalactic supernovae to measure shock deceleration and test explosion mechanisms.
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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Unraveling the mysteries of supernovae with SKA+VLBI
SKA+VLBI will enable routine mas-scale imaging of nearby extragalactic supernovae to measure shock deceleration and test explosion mechanisms.