The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence Layering

Volcanic ash clouds often become multilayered and thin with distance from the vent. We explore one mechanism for the development of this layered structure. We review data on the characteristics of turbulence layering in the free atmosphere, as well as examples of observations of layered clouds both...

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Main Authors: Marcus Bursik, Qingyuan Yang, Adele Bear-Crozier, Michael Pavolonis, Andrew Tupper
Format: Article
Language:English
Published: MDPI AG 2021-02-01
Series:Atmosphere
Subjects:
Online Access:https://www.mdpi.com/2073-4433/12/2/285
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author Marcus Bursik
Qingyuan Yang
Adele Bear-Crozier
Michael Pavolonis
Andrew Tupper
author_facet Marcus Bursik
Qingyuan Yang
Adele Bear-Crozier
Michael Pavolonis
Andrew Tupper
author_sort Marcus Bursik
collection DOAJ
description Volcanic ash clouds often become multilayered and thin with distance from the vent. We explore one mechanism for the development of this layered structure. We review data on the characteristics of turbulence layering in the free atmosphere, as well as examples of observations of layered clouds both near-vent and distally. We then explore dispersion models that explicitly use the observed layered structure of atmospheric turbulence. The results suggest that the alternation of turbulent and quiescent atmospheric layers provides one mechanism for the development of multilayered ash clouds by modulating vertical particle motion. The largest particles, generally <inline-formula>μ<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>></mo><mn>100</mn><mo> </mo><mi mathvariant="sans-serif">μ</mi></mrow></semantics></math></inline-formula>m, are little affected by turbulence. For particles in which both settling and turbulent diffusion are important to vertical motion, mostly in the range of 10–100 <inline-formula>μ<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">μ</mi></semantics></math></inline-formula>m, the greater turbulence intensity and more rapid turbulent diffusion in some layers causes these particles to spend greater time in the more turbulent layers, leading to a layering of concentration. The results may have important implications for ash cloud forecasting and aviation safety.
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spelling doaj.art-7b9ba7ac3e7a4da6bb420b690205b4892023-12-11T18:04:41ZengMDPI AGAtmosphere2073-44332021-02-0112228510.3390/atmos12020285The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence LayeringMarcus Bursik0Qingyuan Yang1Adele Bear-Crozier2Michael Pavolonis3Andrew Tupper4Center for Geohazards Studies, University at Buffalo, Buffalo, NY 14260, USAEarth Observatory of Singapore and Asian School of the Environment, Nanyang Technological University, Singapore 639798, SingaporeBureau of Meteorology, Melbourne, VIC 3001, AustraliaNOAA Cooperative Institute for Meteorological Satellite Studies, University of Wisconsin, Madison, WI 53706, USANatural Hazards Consulting, Montmorency, VIC 3094, AustraliaVolcanic ash clouds often become multilayered and thin with distance from the vent. We explore one mechanism for the development of this layered structure. We review data on the characteristics of turbulence layering in the free atmosphere, as well as examples of observations of layered clouds both near-vent and distally. We then explore dispersion models that explicitly use the observed layered structure of atmospheric turbulence. The results suggest that the alternation of turbulent and quiescent atmospheric layers provides one mechanism for the development of multilayered ash clouds by modulating vertical particle motion. The largest particles, generally <inline-formula>μ<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>></mo><mn>100</mn><mo> </mo><mi mathvariant="sans-serif">μ</mi></mrow></semantics></math></inline-formula>m, are little affected by turbulence. For particles in which both settling and turbulent diffusion are important to vertical motion, mostly in the range of 10–100 <inline-formula>μ<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">μ</mi></semantics></math></inline-formula>m, the greater turbulence intensity and more rapid turbulent diffusion in some layers causes these particles to spend greater time in the more turbulent layers, leading to a layering of concentration. The results may have important implications for ash cloud forecasting and aviation safety.https://www.mdpi.com/2073-4433/12/2/285turbulenceeddy diffusivityash layervolcanic cloudash cloudPinatubo
spellingShingle Marcus Bursik
Qingyuan Yang
Adele Bear-Crozier
Michael Pavolonis
Andrew Tupper
The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence Layering
Atmosphere
turbulence
eddy diffusivity
ash layer
volcanic cloud
ash cloud
Pinatubo
title The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence Layering
title_full The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence Layering
title_fullStr The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence Layering
title_full_unstemmed The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence Layering
title_short The Development of Volcanic Ash Cloud Layers over Hours to Days Due to Atmospheric Turbulence Layering
title_sort development of volcanic ash cloud layers over hours to days due to atmospheric turbulence layering
topic turbulence
eddy diffusivity
ash layer
volcanic cloud
ash cloud
Pinatubo
url https://www.mdpi.com/2073-4433/12/2/285
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