Atmospheric Kelvin–Helmholtz billows captured by the MU radar, lidars and a fish-eye camera
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- Material Type
- 記事
- Author/Editor
- Hubert LuceLakshmi KanthaMasanori 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
- DOI
- 10.1186/s40623-018-0935-0
- Persistent ID (NDL)
- info:ndljp/pid/11189224
- Collection
- 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
- 可
- Periodical Title (URI)
- 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
- 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.
- DOI
- 10.1186/s40623-018-0935-0
- 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.
- Related Material (URI)
- 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 resultsExtensive studies of large‐amplitude Kelvin–Helmholtz billows in the lower atmosphere with VHF middle and upper atmosphere radarConvective Instability Underneath Midlevel Clouds: Comparisons between Numerical Simulations and VHF Radar ObservationsThe Mysteries of Mammatus Clouds: Observations and Formation MechanismsFactors Governing Cellular Convection in Orographic PrecipitationMicro pulse lidarObservations of Kelvin‐Helmholtz instability at a cloud base with the middle and upper atmosphere (MU) and weather radarsHigh-Resolution Observations with MU Radar of a KH Instability Triggered by an Inertia–Gravity Wave in the Upper Part of a Jet StreamEvolution and Breakdown of Kelvin–Helmholtz Billows in Stratified Compressible Flows. Part I: Comparison of Two- and Three-Dimensional FlowsEnergetics of persistent turbulent layers underneath mid-level clouds estimated from concurrent radar and radiosonde dataFurther study of a jet stream‐generated Kelvin‐Helmholtz instabilityExperiments on instability and turbulence in a stratified shear flowCombined temperature lidar for measurements in the troposphere, stratosphere, and mesosphereRetrieving Cloud Characteristics from Ground-Based Daytime Color All-Sky ImagesSpace and Time Filtering of Remotely Sensed Velocity TurbulenceOn the Effects of Moisture on the Brunt-Väisälä FrequencyA frequency domain radar interferometric imaging (FII) technique based on high-resolution methodsTurbulence statistics of a Kelvin–Helmholtz billow event observed in the night-time boundary layer during the Cooperative Atmosphere–Surface Exchange Study field programRange imaging using frequency diversityFull-Time, Eye-Safe Cloud and Aerosol Lidar Observation at Atmospheric Radiation Measurement Program Sites: Instruments and Data ProcessingMidlatitude Cirrus Clouds Derived from Hurricane Nora: A Case Study with Implications for Ice Crystal Nucleation and ShapeMU radar: New capabilities and system calibrations
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 学術機関リポジトリデータベース雑誌記事索引データベースCrossrefCiNii Articles科学研究費助成事業データベース科学研究費助成事業データベースCrossrefCrossref
- Bibliographic ID (NDL)
- 11189224
- NAID
- 120006892065