Modified MLT on Hinode blue continuum images yields 70-90 km smaller median UD diameters and 12-13% fill fractions versus 17-19% for regular MLT, with nearly identical intensity histograms and spatial clustering.
II: Some Properties of Umbral Dots
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A visual transformer model trained on IRIS inversions predicts chromospheric temperature and density from SDO data with correlations around 0.8 on 80% of test cases.
citing papers explorer
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A Modified Multi-Level Tracking Scheme for the Detection of Sunspot Umbral Dots
Modified MLT on Hinode blue continuum images yields 70-90 km smaller median UD diameters and 12-13% fill fractions versus 17-19% for regular MLT, with nearly identical intensity histograms and spatial clustering.
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Predicting the thermodynamics in the chromosphere from the translation of SDO data into the IRIS$^{2}$ inversion results using a visual transformer model
A visual transformer model trained on IRIS inversions predicts chromospheric temperature and density from SDO data with correlations around 0.8 on 80% of test cases.