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This 29-minute conference talk by Pravabati Chingangbam explores how morphological statistics can be used to probe the universe through 21cm brightness temperature measurements. Delivered at the International Centre for Theoretical Sciences as part of the "Radio Cosmology and Continuum Observations in the SKA Era: A Synergic View" program, the presentation contributes to discussions about the Square Kilometre Array (SKA) telescope project scheduled to begin operations in 2027. Learn about advanced techniques for analyzing cosmic structures through statistical methods that reveal patterns in 21cm signals. This talk is part of a two-week program bringing together experts in radio cosmology and continuum science, designed to foster collaboration and train the next generation of researchers in preparation for the SKA, which will be one of the greatest scientific and engineering achievements of the 21st century.
