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Clear Air Turbulence Observed Across a Tropopause Fold Over the Drake Passage-A Case Study
Indexado
WoS WOS:000765621000030
Scopus SCOPUS_ID:85127787923
DOI 10.1029/2021JD035908
Año 2022
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



An aircraft turbulence encounter over the Drake Passage is investigated by combining unique high-frequency flight level data, vertical profiles of a near-simultaneous radiosonde profile and numerical results from global and regional numerical weather prediction (NWP) models. Meteorological analysis reveals an intense polar low propagating from the Bellinghausen Sea toward the Drake Passage. A small and deep stratospheric intrusion formed a tropopause fold that promoted strong upper-level frontogenesis and enhanced shear and horizontal deformation of the upper tropospheric and lower stratospheric (UTLS) airflow. In this region, the Basic HALO Measurement and Sensor System (BAHAMAS) aboard the HALO research aircraft flying at FL450 detected large peak-to-peak variations in all meteorological parameters. The computed Energy dissipation rate (EDR) values (cubic root of the eddy dissipation rate) indicate moderate to severe turbulence. The location of this turbulence encounter was well-predicted by the clear air turbulence (CAT) indices derived from the NWP results. The enhanced CAT indices emphasize the large shear and horizontal deformation of the airflow as the cause of the turbulence. Horizontal and vertical energy spectra calculated from the 10 Hz BAHAMAS data show a well-defined energy cascade toward small scales with Kolmogorov scaling. Maximum EDR values of about 0.35 derived both from the spectra and structure functions for the wind speed agree quantitatively very well. In addition, the structure functions support the detection of turbulent atmospheric conditions with signatures of flow anisotropy generated by enhanced thermal stratification in the UTLS. The scales involved are between the buoyancy length scale L-B approximate to 1,500 m and the Ozmidov scale L-O approximate to 111 m.

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Disciplinas de Investigación



WOS
Meteorology & Atmospheric Sciences
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Rodriguez Imazio, Paola Mujer Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
Serv Meteorol Nacl - Argentina
Consejo Nacional de Investigaciones Científicas y Técnicas - Argentina
Ministerio de Defensa República Argentina - Argentina
2 Doernbrack, Andreas Hombre Inst Phys Atmosphare - Alemania
Deutsches Zentrum für Luft- und Raumfahrt (DLR) - Alemania
3 Delgado Urzua, Rodrigo Hombre Direcc Meteorol Chile - Chile
Direccion Meteorologica de Chile - Chile
3 Urzua, Rodrigo Delgado Hombre Direccion Meteorologica de Chile - Chile
Direcc Meteorol Chile - Chile
4 Rivaben, Nicolas Hombre Serv Meteorol Nacl - Argentina
Ministerio de Defensa República Argentina - Argentina
5 GODOY-SANCHEZ, ALEJANDRO SAMUEL Hombre Serv Meteorol Nacl - Argentina
Ministerio de Defensa República Argentina - Argentina

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Financiamiento



Fuente
Bundesministerium für Bildung und Forschung
Argentinian Ministry of Defense
German research initiative "Role of the middle atmosphere in climate" (ROMIC) under Federal Ministry for Education and Research

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
This work was supported by the project PIDDEF ESP 2/2018 granted by the Argentinian Ministry of Defense. P. Rodriguez Imazio will like to thank Pablo Mininni for a thoughtful discussion and probing questions, and Luciano Vidal and Martin Rugna for assistance on satellite images. This research was partly funded by the German research initiative "Role of the middle atmosphere in climate" (ROMIC) under grant 01LG1206A provided by the Federal Ministry for Education and Research.
This work was supported by the project PIDDEF ESP 2/2018 granted by the Argentinian Ministry of Defense. P. Rodriguez Imazio will like to thank Pablo Mininni for a thoughtful discussion and probing questions, and Luciano Vidal and Martin Rugna for assistance on satellite images. This research was partly funded by the German research initiative “Role of the middle atmosphere in climate” (ROMIC) under grant 01LG1206A provided by the Federal Ministry for Education and Research.

Muestra la fuente de financiamiento declarada en la publicación.