Received: 3 May 2019 Revised: 29 October 2019 Accepted: 8 November 2019 DOI: 10.1002/qj.3701 RESEARCH ARTICLE An idealized numerical study of tropical cyclogenesis and evolution at the Equator Gerard Kilroy1 Roger K. Smith1 Michael T. Montgomery2 1Meteorological Institute, Ludwig-Maximilians University of Abstract Munich, Munich, Germany Tropical cyclone formation and evolution at, or near, the Equator is explored 2Department of Meteorology, Naval using idealized three-dimensional model simulations, starting from a pre- Postgraduate School, Monterey, California scribed, initial, weak counterclockwise rotating vortex in an otherwise quies- Correspondence cent, nonrotating environment. Three simulations are carried out in which the G. Kilroy, Meteorological Institute, maximum tangential wind speed (5 m s−1) is specified at an initial radius of 50, Ludwig-Maximilians University of Munich, Theresienstr. 37, 80333 Munich, 100, or 150 km. After a period of gestation lasting between 30 and 60 hr, the vor- Germany. tices intensify rapidly, the evolution being similar to that for vortices away from Email:
[email protected] the Equator. In particular, the larger the initial vortex size, the longer the gesta- Funding information tion period, the larger the maximum intensity attained, and the longer the vortex Deutsche Forschungsgemeinschaft, KO lifetime. Beyond a few days, the vortices decay as the cyclonic vorticity source 2248/2-1; National Science Foundation, provided by the initial vortex is depleted and negative vorticity surrounding the AGS-1313948; Office of Naval Research, vortex core is drawn inwards by the convectively driven overturning circulation. N0001417WX00336 In these negative vorticity regions, the flow is inertially/centrifugally unstable. The vortex evolution during the mature and decay phases differs from that in simulations away from the Equator, where inertially unstable regions are much more limited in area.