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電子書籍・電子雑誌EPS : Earth, Planets and Space
Volume number70
Atmospheri...

Atmospheric Kelvin–Helmholtz billows captured by the MU radar, lidars and a fish-eye camera

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Atmospheric Kelvin–Helmholtz billows captured by the MU radar, lidars and a fish-eye camera

Call No. (NDL)
Z18-B377
Bibliographic ID of National Diet Library
11189224
Persistent ID (NDL)
info:ndljp/pid/11189224
Material type
記事
Author
Hubert Luceほか
Publisher
Springer Nature
Publication date
2018-10-03
Material Format
Paper・Digital
Journal name
EPS : Earth, Planets and Space 70(162)
Publication Page
-
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On June 11, 2015, a train of large-amplitude Kelvin–Helmholtz (KH) billows was monitored by the Middle and Upper Atmosphere (MU) radar (Shigaraki MU O...

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Digital

Material Type
記事
Author/Editor
Hubert Luce
Lakshmi Kantha
Masanori Yabuki
Publication, Distribution, etc.
Publication Date
2018-10-03
Publication Date (W3CDTF)
2018-10-03
Periodical title
EPS : Earth, Planets and Space
No. or year of volume/issue
70(162)
Volume
70(162)
ISSN (Periodical Title)
1880-5981
ISSN-L (Periodical Title)
1343-8832
Text Language Code
eng
Persistent ID (NDL)
info:ndljp/pid/11189224
Collection (Materials For Handicapped People:1)
Collection (particular)
国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
Acquisition Basis
オンライン資料収集制度
Date Accepted (W3CDTF)
2018-11-22T14:07:23+09:00
Date Captured (W3CDTF)
2018-11-21
Format (IMT)
application/pdf
Access Restrictions
国立国会図書館内限定公開
Service for the Digitized Contents Transmission Service
図書館・個人送信対象外
Availability of remote photoduplication service
Periodical Title (Persistent ID (NDL))
info:ndljp/pid/11067456
Data Provider (Database)
国立国会図書館 : 国立国会図書館デジタルコレクション

Digital

Summary, etc.
On June 11, 2015, a train of large-amplitude Kelvin–Helmholtz (KH) billows was monitored by the Middle and Upper Atmosphere (MU) radar (Shigaraki MU Observatory, Japan) at the altitude of ~ 6.5 km. Four to five KH billows in formation and decay stages were observed for about 20 min at the height of a strong speed shear (> ~ 30 m s⁻¹km⁻¹), just a few hundred meters above a mid-level cloud base. The turbulent billows had a spacing of about 3.5–4.0 km (3.71 km in average) and an aspect ratio (depth/spacing) of ~ 0.3. The turbulence kinetic energy dissipation rate estimated was of the order of 10–50 mWkg⁻¹, corresponding to moderate turbulence according to ICAO (2010) classification. By chance, an upward-looking fish-eye camera producing pictures once every minute detected smooth protuberances at the cloud base caused by the KH billows so that comparisons of their characteristics could be made for the first time between the radar observations and the pictures. The main characteristics of the KH wave (horizontal wavelength, phase front direction and phase speed) obtained from the analysis of the pictures were fully consistent with those found from radar data. The pictures indicated that the billows were advected by the wind observed at the height of the critical level. They also revealed a very small transverse extent (about twice the horizontal spacing) suggesting that the large-amplitude KH billows were generated by a very localized source. Micro-pulse lidar and Raman–Rayleigh–Mie lidar data also collected during the event permitted us to confirm some of the characteristics of the billows.
Access Restrictions
インターネット公開
Rights (production)
© The Author(s) 2018. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
Is Referenced By
Special issue “Recent Advances in MST and EISCAT/Ionospheric Studies – Special Issue of the Joint MST15 and EISCAT18 Meetings, May 2017”
New cloud morphologies discovered on the Venus's night during Akatsuki
References
Shigaraki UAV-Radar Experiment (ShUREX): overview of the campaign with some preliminary results
Extensive studies of large‐amplitude Kelvin–Helmholtz billows in the lower atmosphere with VHF middle and upper atmosphere radar
Convective Instability Underneath Midlevel Clouds: Comparisons between Numerical Simulations and VHF Radar Observations
The Mysteries of Mammatus Clouds: Observations and Formation Mechanisms
Factors Governing Cellular Convection in Orographic Precipitation
Micro pulse lidar
Observations of Kelvin‐Helmholtz instability at a cloud base with the middle and upper atmosphere (MU) and weather radars
High-Resolution Observations with MU Radar of a KH Instability Triggered by an Inertia–Gravity Wave in the Upper Part of a Jet Stream
Evolution and Breakdown of Kelvin–Helmholtz Billows in Stratified Compressible Flows. Part I: Comparison of Two- and Three-Dimensional Flows
Energetics of persistent turbulent layers underneath mid-level clouds estimated from concurrent radar and radiosonde data
Further study of a jet stream‐generated Kelvin‐Helmholtz instability
Experiments on instability and turbulence in a stratified shear flow
Combined temperature lidar for measurements in the troposphere, stratosphere, and mesosphere
Retrieving Cloud Characteristics from Ground-Based Daytime Color All-Sky Images
Space and Time Filtering of Remotely Sensed Velocity Turbulence
On the Effects of Moisture on the Brunt-Väisälä Frequency
A frequency domain radar interferometric imaging (FII) technique based on high-resolution methods
Turbulence statistics of a Kelvin–Helmholtz billow event observed in the night-time boundary layer during the Cooperative Atmosphere–Surface Exchange Study field program
Range imaging using frequency diversity
Full-Time, Eye-Safe Cloud and Aerosol Lidar Observation at Atmospheric Radiation Measurement Program Sites: Instruments and Data Processing
Midlatitude Cirrus Clouds Derived from Hurricane Nora: A Case Study with Implications for Ice Crystal Nucleation and Shape
MU radar: New capabilities and system calibrations
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国立情報学研究所 : CiNii Research
Original Data Provider (Database)
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Bibliographic ID (NDL)
11189224
NAID
120006892065