Firn Densification: An Empirical Model

Abstract An empirical model of firn densification from the surface to the zone of pore close-off has been constructed. Fundamental rate equations have been derived for the first two stages of densification. In the first stage, for densities less than 0.55 Mg m −3 , the densification rate is proporti...

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Bibliographic Details
Published in:Journal of Glaciology
Main Authors: Herron, Michael M., Langway, Chester C.
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 1980
Subjects:
Online Access:http://dx.doi.org/10.1017/s0022143000015239
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0022143000015239
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Summary:Abstract An empirical model of firn densification from the surface to the zone of pore close-off has been constructed. Fundamental rate equations have been derived for the first two stages of densification. In the first stage, for densities less than 0.55 Mg m −3 , the densification rate is proportional to the mean annual accumulation times the term ( ρ i − ρ ), where ρ is the density of the snow and ρ i is the density of pure ice. The densification rate in the second stage, where 0.55 Mg m −3 < ρ < 0.8 Mg m −3 , is proportional to the square root of the accumulation rate and to ( ρ i− ρ ). Depth–density and depth–age calculations from this model are compared with observation. Model accumulation rates are within about 20% of values obtained by other techniques. It is suggested that depth intervals of constant density in some Antarctic cores may represent a synchronous event in the 1880 ’s when ten times the normal accumulation fell within a year or two.