Buoyancy of Convective Vertical Motions in the Inner Core of Intense Hurricanes. Part I: General Statistics
Open Access
- 1 January 2005
- journal article
- Published by American Meteorological Society in Monthly Weather Review
- Vol. 133 (1) , 188-208
- https://doi.org/10.1175/mwr-2848.1
Abstract
The buoyancy of hurricane convective vertical motions is studied using aircraft data from 175 radial legs collected in 14 intense hurricanes at four altitudes ranging from 1.5 to 5.5 km. The data of each leg are initially filtered to separate convective-scale features from background mesoscale structure. Convective vertical motion events, called cores, are identified using the criteria that the convective-scale vertical velocity must exceed 1.0 m s−1 for at least 0.5 km. A total of 620 updraft cores and 570 downdraft cores are included in the dataset. Total buoyancy is calculated from convective-scale virtual potential temperature, pressure, and liquid water content using the mesoscale structure as the reference state. Core properties are summarized for the eyewall and rainband regions at each altitude. Characteristics of core average convective vertical velocity, maximum convective vertical velocity, and diameter are consistent with previous studies of hurricane convection. Most cores are superimposed upon relatively weak mesoscale ascent. The mean eyewall (rainband) updraft core exhibits small, but statistically significant, positive total buoyancy below 4 km (between 2 and 5 km) and a modest increase in vertical velocity with altitude. The mean downdraft core not superimposed upon stronger mesoscale ascent also exhibits positive total buoyancy and a slight decrease in downward vertical velocity with decreasing altitude. Buoyant updraft cores cover less than 5% of the total area in each region but accomplish ∼40% of the total upward transport. A one-dimensional updraft model is used to elucidate the relative roles played by buoyancy, vertical perturbation pressure gradient forces, water loading, and entrainment in the vertical acceleration of ordinary updraft cores. Small positive total buoyancy values are found to be more than adequate to explain the vertical accelerations observed in updraft core strength, which implies that ordinary vertical perturbation pressure gradient forces are directed downward, opposing the positive buoyancy forces. Entrainment and water loading are also found to limit updraft magnitudes. The observations support some aspects of both the hot tower hypothesis and symmetric moist neutral ascent, but neither concept appears dominant. Buoyant convective updrafts, however, are integral components of the hurricane’s transverse circulation.Keywords
This publication has 61 references indexed in Scilit:
- Buoyancy of Convective Vertical Motions in the Inner Core of Intense Hurricanes. Part II: Case StudiesMonthly Weather Review, 2005
- Some Views On “Hot Towers” after 50 Years of Tropical Field Programs and Two Years of TRMM DataPublished by Springer Nature ,2003
- Buoyancy of Convective Clouds in TOGA COAREJournal of the Atmospheric Sciences, 1998
- Thermals with background rotation and stratificationJournal of Fluid Mechanics, 1994
- Mesoscale and Convective-Scale Characteristics of Mature Hurricanes. Part II. Inner Core Structure of Hurricane Allen (1980)Journal of the Atmospheric Sciences, 1984
- An Analysis and Comparison of Five Water Droplet Measuring InstrumentsJournal of Climate and Applied Meteorology, 1983
- Forced secondary circulations in hurricanesJournal of Geophysical Research: Oceans, 1979
- Cloud Patterns in Hurricane Daisy, 1958Tellus A: Dynamic Meteorology and Oceanography, 1961
- Some Aspects of Hurricane Daisy, 1958Tellus A: Dynamic Meteorology and Oceanography, 1961
- On the Dynamics and Energy Transformations in Steady-State HurricanesTellus A: Dynamic Meteorology and Oceanography, 1960