Large eddy simulation of dust devils in a diurnally-evolving convective mixed layer

Junshi Ito, Ryo Tanaka, Hiroshi Niino, Mikio Nakanishi

研究成果: Article査読

17 被引用数 (Scopus)

抄録

Formation of dust devils in diurnally-evolving convective mixed layers is studied by means of a large eddy simulation. It is found that a weaker general wind and a stronger surface heat flux for which cellular convection rather than roll convection prevails are favorable for the formation of dust devils. The simulation results show that when the general wind is weak, the maximum vertical vorticity in the convective mixed layer is a monotonically increasing function of w*, where w* is the convective velocity scale for a convective mixed layer. Therefore, dust devils occur most frequently in the early afternoon when the heat flux is large and the convective mixed layer grows to a significant height. The simulated dust devils are found to have a horizontal length scale comparable with observed larger dust devils. They have either one-celled or two-celled structure. Some of them have a one-celled structure initially, but later evolve into a two-celled structure.

本文言語English
ページ(範囲)63-77
ページ数15
ジャーナルJournal of the Meteorological Society of Japan
88
1
DOI
出版ステータスPublished - 2010
外部発表はい

ASJC Scopus subject areas

  • Atmospheric Science

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