TY - JOUR
T1 - Statistical Analysis of Convective Updrafts in Tropical Cyclone Rainbands Observed by Airborne Doppler Radar
AU - Barron, Nicholas R.
AU - Didlake, Anthony C.
AU - Reasor, Paul D.
N1 - Funding Information:
We would like to thank George Young, Kelly Lombardo, James Ruppert, Frank Marks, and three anonymous reviewers for their comments and suggestions on this work. We are grateful for Beth Tully and her work on the conceptual model, the last of her excellent contributions to scientific literature in the past 18 years. We would also like to thank John Gamache and Michael Fischer for developing and maintaining the TDR analysis dataset at HRD. We also thank NOAA’s Aircraft Operations Center staff, who have collected the TDR data over many years and made such multi‐case studies possible. This material is based upon work supported by the National Science Foundation under Award No. AGS‐1810869. Any opinions, findings, and conclusions or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.
Publisher Copyright:
© 2022. American Geophysical Union. All Rights Reserved.
PY - 2022/3/27
Y1 - 2022/3/27
N2 - Ten years of airborne Doppler radar observations are used to study convective updrafts' kinematic and reflectivity structures in tropical cyclone (TC) rainbands. An automated algorithm is developed to identify the strongest rainband updrafts across 12 hurricane-strength TCs. The selected updrafts are then collectively analyzed by their frequency, radius, azimuthal location (relative to the 200–850 hPa environmental wind shear), structural characteristics, and secondary circulation (radial/vertical) flow pattern. Rainband updrafts become deeper and stronger with increasing radius. A wavenumber-1 asymmetry arises, showing that in the downshear (upshear) quadrants of the TC, updrafts are more (less) frequent and deeper (shallower). In the downshear quadrants, updrafts primarily have in-up-out or in-up-in secondary circulation patterns. The in-up-out circulation is the most frequent pattern and has the deepest updraft and reflectivity tower. Upshear, the updrafts generally have out-up-in or in-up-in patterns. The radial flow of the updraft circulations largely follows the vortex-scale radial flow shear-induced asymmetry, being increased low-level inflow (outflow) and midlevel outflow (inflow) in the downshear (upshear) quadrants. It is hypothesized that the convective-scale circulations are significantly influenced by the vortex-scale radial flow at the updraft base and top altitudes. Other processes of the convective life cycle, such as bottom-up decay of aging convective updrafts due to increased low-level downdrafts, can influence the base altitude and, thus, the base radial flow of the updraft circulation. The findings presented in this study support previous literature regarding convective-scale patterns of organized rainband convection in a mature, sheared TC.
AB - Ten years of airborne Doppler radar observations are used to study convective updrafts' kinematic and reflectivity structures in tropical cyclone (TC) rainbands. An automated algorithm is developed to identify the strongest rainband updrafts across 12 hurricane-strength TCs. The selected updrafts are then collectively analyzed by their frequency, radius, azimuthal location (relative to the 200–850 hPa environmental wind shear), structural characteristics, and secondary circulation (radial/vertical) flow pattern. Rainband updrafts become deeper and stronger with increasing radius. A wavenumber-1 asymmetry arises, showing that in the downshear (upshear) quadrants of the TC, updrafts are more (less) frequent and deeper (shallower). In the downshear quadrants, updrafts primarily have in-up-out or in-up-in secondary circulation patterns. The in-up-out circulation is the most frequent pattern and has the deepest updraft and reflectivity tower. Upshear, the updrafts generally have out-up-in or in-up-in patterns. The radial flow of the updraft circulations largely follows the vortex-scale radial flow shear-induced asymmetry, being increased low-level inflow (outflow) and midlevel outflow (inflow) in the downshear (upshear) quadrants. It is hypothesized that the convective-scale circulations are significantly influenced by the vortex-scale radial flow at the updraft base and top altitudes. Other processes of the convective life cycle, such as bottom-up decay of aging convective updrafts due to increased low-level downdrafts, can influence the base altitude and, thus, the base radial flow of the updraft circulation. The findings presented in this study support previous literature regarding convective-scale patterns of organized rainband convection in a mature, sheared TC.
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U2 - 10.1029/2021JD035718
DO - 10.1029/2021JD035718
M3 - Article
AN - SCOPUS:85127360850
SN - 2169-897X
VL - 127
JO - Journal of Geophysical Research: Atmospheres
JF - Journal of Geophysical Research: Atmospheres
IS - 6
M1 - e2021JD035718
ER -