## Abstract The interaction of vortex patches in relation to the observed scales and features reported in Part I of this paper is investigated. It is found that the initial approach of compound vortices, such as tropical cyclones, arises from distortion of their, weaker, outer vorticity fields. Car
On the interaction of tropical-cyclone-scale vortices. I: Observations
✍ Scribed by Mark Lander; Greg J. Holland
- Publisher
- John Wiley and Sons
- Year
- 1993
- Tongue
- English
- Weight
- 879 KB
- Volume
- 119
- Category
- Article
- ISSN
- 0035-9009
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✦ Synopsis
Abstract
A detailed analysis is made of the observed behaviour in interaction, tropical‐cyclone‐scale vortices in the western North Pacific region. It is found that all multiple‐vortex interactions can be broken down into a common model of binary interaction. The classical Fujiwhara model of converging cyclonic rotation about a centroid followed by merger is rarely followed. Capture tends to occur rapidly, within several hours, and is followed by a period of relatively stable cyclonic orbit. Cyclone merger occurs by one vortex experiencing a loss of convective organization, followed by horizontal shearing and incorporation into the outer circulation of the other vortex. However, a substantial proportion of interacting cyclones escape from the interaction, and the changeover from a stable orbiting configuration occurs rapidly. A model of binary interaction is presented.
Cases where swarms of mesoscale vortices are formed in convectively active regions without tropical cyclones are also documented. These vortices have a much narrower range of influence (a few hundred kilometres) then that observed for tropical cyclones. When groups of vortices come within this range they are observed to conform to the same interaction model as observed for tropical cyclones.
📜 SIMILAR VOLUMES
Ab initio extcnsivc configuration interaction calculations were wrried out on the n-electron stsies of benzene. Among the three = -+ T;\*(elg+ e,,) sinplet states, 'BzU(SI). 'B1,(SI), and 'El, (S ), the TY\* orbital WZF found tc 3 b2 valence-like in S, and Sz, but diffuse in S3. All three correspon