Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/5401
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dc.contributor.authorAli, Imamah-
dc.contributor.authorOsuri, Krishna Kishore-
dc.date.accessioned2025-12-11T12:51:07Z-
dc.date.available2025-12-11T12:51:07Z-
dc.date.issued2025-11-
dc.identifier.citationInternational Symposium on Tropical Meteorology (INTROMET), IITM, Pune, 18-20 November 2025en_US
dc.identifier.urihttp://hdl.handle.net/2080/5401-
dc.descriptionCopyright belongs to the proceeding publisher.en_US
dc.description.abstractMonsoon depressions (MDs) are the significant synoptic systems over the Indian monsoon region, accounting for a substantial fraction (two-thirds) of the seasonal rainfall and associated hazards. Despite their importance, systematic evaluations of MD structure in high-resolution NWP models remain limited. Here, we simulated ten MD cases using an ARW-WRF model (resolution d01 : 13.5, d02 : 4.5 km nested domains) and evaluated storm-centric composites against ERA5 reanalysis and GPM across 24–60 h lead times. Track and rainfall errors are modest at early lead times and increase gradually with forecast length; track deviations rise slowly with time, while rainfall skill degrades from 24 to 60 hours, with strong overprediction near the storm center, weakening outward with a negative bias on the southern flank. Near-surface (10 m) winds remain nearly unbiased for about two days; uncertainty increases at longer lead times. Despite these errors, the model still reproduces the canonical MD structure, including the low-level cyclonic circulation, cold-to-warm core transition, and 850-hPa wind field.en_US
dc.subjectMonsoon depressionsen_US
dc.subjectARW-WRF modelen_US
dc.titleAnalysis of the Structure and Dynamics of Monsoon Depression using High Resolution ARW-WRF Modelen_US
dc.typePresentationen_US
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