Home > Research > Publications & Outputs > The influence of shape on the atmospheric settl...
View graph of relations

The influence of shape on the atmospheric settling velocity of volcanic ash particles

Research output: Contribution to journalJournal articlepeer-review

Published

Standard

The influence of shape on the atmospheric settling velocity of volcanic ash particles. / Wilson, L.; Huang, T. C.

In: Earth and Planetary Science Letters, Vol. 44, No. 2, 01.08.1979, p. 311-324.

Research output: Contribution to journalJournal articlepeer-review

Harvard

APA

Vancouver

Author

Wilson, L. ; Huang, T. C. / The influence of shape on the atmospheric settling velocity of volcanic ash particles. In: Earth and Planetary Science Letters. 1979 ; Vol. 44, No. 2. pp. 311-324.

Bibtex

@article{356b9021dfb74a4da5f3d9e887c18208,
title = "The influence of shape on the atmospheric settling velocity of volcanic ash particles",
abstract = "Experimental measurements of terminal fall velocities at sea level are reported for pumices, glass shards, and feldspar crystals with mean diameters between 30 and >500 μm. The velocities depend significantly on particle shape and rotation mode as well as density and size. Six tumbling modes were observed, of which two are predominant. The measurements have been converted to drag coefficients and Reynolds numbers so that they can be used to compute terminal velocities at any height in the atmosphere. It was found that if the drag coefficient and Reynolds number are defined empirically in terms of the arithmetic mean particle diameter, the effects of shape and rotation can be fully accounted for by defining a shape parameter, F, for each particle. In terms of the lengths of the longest, intermediate and shortest principal axes of the particle, denoted a, b, and c, respectively, F = (b + c) 2a. A simple formula for the drag coefficient, Ca, as a function of Reynolds number, Ra, and shape parameter is: Ca= 24 RaF-0.828+2 1.07-F. A more fundamental analysis allows the measurements made here to be compared with theoretical curves and experimental data on simple particle shapes from wind tunnel studies.",
author = "L. Wilson and Huang, {T. C.}",
year = "1979",
month = aug,
day = "1",
doi = "10.1016/0012-821X(79)90179-1",
language = "English",
volume = "44",
pages = "311--324",
journal = "Earth and Planetary Science Letters",
issn = "0012-821X",
publisher = "Elsevier Science B.V.",
number = "2",

}

RIS

TY - JOUR

T1 - The influence of shape on the atmospheric settling velocity of volcanic ash particles

AU - Wilson, L.

AU - Huang, T. C.

PY - 1979/8/1

Y1 - 1979/8/1

N2 - Experimental measurements of terminal fall velocities at sea level are reported for pumices, glass shards, and feldspar crystals with mean diameters between 30 and >500 μm. The velocities depend significantly on particle shape and rotation mode as well as density and size. Six tumbling modes were observed, of which two are predominant. The measurements have been converted to drag coefficients and Reynolds numbers so that they can be used to compute terminal velocities at any height in the atmosphere. It was found that if the drag coefficient and Reynolds number are defined empirically in terms of the arithmetic mean particle diameter, the effects of shape and rotation can be fully accounted for by defining a shape parameter, F, for each particle. In terms of the lengths of the longest, intermediate and shortest principal axes of the particle, denoted a, b, and c, respectively, F = (b + c) 2a. A simple formula for the drag coefficient, Ca, as a function of Reynolds number, Ra, and shape parameter is: Ca= 24 RaF-0.828+2 1.07-F. A more fundamental analysis allows the measurements made here to be compared with theoretical curves and experimental data on simple particle shapes from wind tunnel studies.

AB - Experimental measurements of terminal fall velocities at sea level are reported for pumices, glass shards, and feldspar crystals with mean diameters between 30 and >500 μm. The velocities depend significantly on particle shape and rotation mode as well as density and size. Six tumbling modes were observed, of which two are predominant. The measurements have been converted to drag coefficients and Reynolds numbers so that they can be used to compute terminal velocities at any height in the atmosphere. It was found that if the drag coefficient and Reynolds number are defined empirically in terms of the arithmetic mean particle diameter, the effects of shape and rotation can be fully accounted for by defining a shape parameter, F, for each particle. In terms of the lengths of the longest, intermediate and shortest principal axes of the particle, denoted a, b, and c, respectively, F = (b + c) 2a. A simple formula for the drag coefficient, Ca, as a function of Reynolds number, Ra, and shape parameter is: Ca= 24 RaF-0.828+2 1.07-F. A more fundamental analysis allows the measurements made here to be compared with theoretical curves and experimental data on simple particle shapes from wind tunnel studies.

U2 - 10.1016/0012-821X(79)90179-1

DO - 10.1016/0012-821X(79)90179-1

M3 - Journal article

AN - SCOPUS:0018736526

VL - 44

SP - 311

EP - 324

JO - Earth and Planetary Science Letters

JF - Earth and Planetary Science Letters

SN - 0012-821X

IS - 2

ER -