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Density‐driven transport in the umbrella region of volcanic clouds: Implications for tephra dispersion models
Author(s) -
Costa Antonio,
Folch Arnau,
Macedonio Giovanni
Publication year - 2013
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/grl.50942
Subject(s) - advection , gravity current , tephra , geology , volcano , buoyancy , volcanic ash , atmospheric sciences , geophysics , atmosphere (unit) , mass transport , environmental science , meteorology , mechanics , physics , seismology , internal wave , oceanography , thermodynamics , engineering physics
Large explosive volcanic eruptions can generate ash clouds from rising plumes that spread in the atmosphere around a Neutral Buoyancy Level (NBL). These ash clouds spread as inertial intrusions and are advected by atmospheric winds. For low mass flow rates, tephra transport is mainly dictated by wind advection, because ash cloud spreading due to gravity current effects is negligible (passive transport). For large mass flow rates, gravity‐driven transport at the NBL can be the dominant transport mechanism. Conditions under which the passive transport assumption is valid have not yet been critically studied. We analyze the conditions when gravity‐driven transport is dominant in terms of the cloud Richardson number. Moreover, we couple an analytical model that describes cloud spreading as a gravity current with an advection‐diffusion model. This coupled model is used to simulate the evolution of the volcanic cloud during the climatic phase of the 1991 Pinatubo eruption.