Toward this end, a climatology of TC inner-core structure is compiled and analyzed. Building upon the research of Piech (2007) and Murray (2009), which gathered and assessed aircraft reconnaissance measurements and compared them to TC intensity changes, satellite measurements from the HURSAT database (Knapp 2008) are used to diagnose TC structure and intensity. An analogue to reconnaissance observations is produced for all worldwide TCs from 1987-2009 using ARCHER software (Wimmers and Velden 2010). From this climatology, patterns of TC structure with respect to location and intensity can be used as an aid to TC prediction. As this climatology is expanded, validation of model performance may eventually reach beyond just track and intensity, but can include TC internal structure as well.
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