MU Radar and Lidar Observations of Clear-Air Turbulence underneath CirrusSource: Monthly Weather Review:;2010:;volume( 138 ):;issue: 002::page 438Author:Luce, Hubert
,
Nakamura, Takuji
,
Yamamoto, Masayuki K.
,
Yamamoto, Mamoru
,
Fukao, Shoichiro
DOI: 10.1175/2009MWR2927.1Publisher: American Meteorological Society
Abstract: Turbulence generation mechanisms prevalent in the atmosphere are mainly shear instabilities, breaking of internal buoyancy waves, and convective instabilities such as thermal convection due to heating of the ground. In the present work, clear-air turbulence underneath a cirrus cloud base is described owing to coincident observations from the VHF (46.5 MHz) middle and upper atmosphere (MU) radar, a Rayleigh?Mie?Raman (RMR) lidar, and a balloon radiosonde on 7?8 June 2006 (at Shigaraki, Japan; 34.85°N, 136.10°E). Time?height cross section of lidar backscatter ratio obtained at 2206 LT 7 June 2006 showed the presence of a cirrus layer between 8.0 and 12.5 km MSL. Downward-penetrating structures of ice crystals with horizontal and vertical extents of 1.0?4.0 km and 200?800 m, respectively, have been detected at the cirrus cloud base for about 35 min. At the same time, the MU radar data revealed clear-air turbulence layers developing downward from the cloud base in the environment of the protuberances detected by the RMR lidar. Their maximum depth was about 2.0 km for about 1.5 h. They were associated with oscillatory vertical wind perturbations of up to ±1.5 m s?1 and variances of Doppler spectrum of 0.2?1.5 m?2 s?2. Analysis of the data suggests that the turbulence and the downward penetration of cloudy air were possibly the consequence of a convective instability (rather than a dynamical shear instability) that was likely due to sublimation of ice crystals in the subcloud region. Downward clear-air motions measured by the MU radar were associated with the descending protuberances, and updrafts were observed between them. These observations suggest that the cloudy air might have been pushed down by the downdrafts of the convective instability and pushed up by the updrafts to form the observed protuberances at the cloud base. These structures may be virga or perhaps more likely mamma as reported by recent observations of cirrus mamma with similar instruments and by numerical simulations.
|
Collections
Show full item record
contributor author | Luce, Hubert | |
contributor author | Nakamura, Takuji | |
contributor author | Yamamoto, Masayuki K. | |
contributor author | Yamamoto, Mamoru | |
contributor author | Fukao, Shoichiro | |
date accessioned | 2017-06-09T16:32:09Z | |
date available | 2017-06-09T16:32:09Z | |
date copyright | 2010/02/01 | |
date issued | 2010 | |
identifier issn | 0027-0644 | |
identifier other | ams-69562.pdf | |
identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4211245 | |
description abstract | Turbulence generation mechanisms prevalent in the atmosphere are mainly shear instabilities, breaking of internal buoyancy waves, and convective instabilities such as thermal convection due to heating of the ground. In the present work, clear-air turbulence underneath a cirrus cloud base is described owing to coincident observations from the VHF (46.5 MHz) middle and upper atmosphere (MU) radar, a Rayleigh?Mie?Raman (RMR) lidar, and a balloon radiosonde on 7?8 June 2006 (at Shigaraki, Japan; 34.85°N, 136.10°E). Time?height cross section of lidar backscatter ratio obtained at 2206 LT 7 June 2006 showed the presence of a cirrus layer between 8.0 and 12.5 km MSL. Downward-penetrating structures of ice crystals with horizontal and vertical extents of 1.0?4.0 km and 200?800 m, respectively, have been detected at the cirrus cloud base for about 35 min. At the same time, the MU radar data revealed clear-air turbulence layers developing downward from the cloud base in the environment of the protuberances detected by the RMR lidar. Their maximum depth was about 2.0 km for about 1.5 h. They were associated with oscillatory vertical wind perturbations of up to ±1.5 m s?1 and variances of Doppler spectrum of 0.2?1.5 m?2 s?2. Analysis of the data suggests that the turbulence and the downward penetration of cloudy air were possibly the consequence of a convective instability (rather than a dynamical shear instability) that was likely due to sublimation of ice crystals in the subcloud region. Downward clear-air motions measured by the MU radar were associated with the descending protuberances, and updrafts were observed between them. These observations suggest that the cloudy air might have been pushed down by the downdrafts of the convective instability and pushed up by the updrafts to form the observed protuberances at the cloud base. These structures may be virga or perhaps more likely mamma as reported by recent observations of cirrus mamma with similar instruments and by numerical simulations. | |
publisher | American Meteorological Society | |
title | MU Radar and Lidar Observations of Clear-Air Turbulence underneath Cirrus | |
type | Journal Paper | |
journal volume | 138 | |
journal issue | 2 | |
journal title | Monthly Weather Review | |
identifier doi | 10.1175/2009MWR2927.1 | |
journal fristpage | 438 | |
journal lastpage | 452 | |
tree | Monthly Weather Review:;2010:;volume( 138 ):;issue: 002 | |
contenttype | Fulltext |