Modeling firn densification through viscosity and microstructures
| dc.contributor.advisor | Waddington, Edwin D | |
| dc.contributor.author | Horlings, Brita Ilyse | |
| dc.date.accessioned | 2020-02-04T19:20:33Z | |
| dc.date.available | 2020-02-04T19:20:33Z | |
| dc.date.issued | 2020-02-04 | |
| dc.date.submitted | 2019 | |
| dc.description | Thesis (Master's)--University of Washington, 2019 | |
| dc.description.abstract | Knowledge of firn densification is important for several applications, such as for ice-sheet surface elevation changes from repeat satellite altimetry methods used to estimate ice-sheet contribution to sea-level rise. Uncertainties in firn-densification rates are among the largest uncertainties for this method mainly because most commonly-used firn-densification models are empirically constructed for estimating the macroscopic behavior of the firn. Currently, no model that is either fully physically-based or is applicable to the entire firn column exists. First, we examine the implicit effective viscosity for models within the Community Firn Model (CFM) under a range of climatic conditions, and find that there exist physically unrealistic discontinuities in viscosity at the transitional density of 550 kg m-3. To generate a continuous viscosity curve, we develop a transition model that gradually transitions processes in zone 1 to those in zone 2 of the firn layer. We use the transition model for estimating depth- density for a range of climates, and we generally see that the transition model shows lower RMSE values compared to the Herron and Langway (1980) model for climatic sites that do not have a regular Clausius-Clapeyron pairing of temperature and accumulation rate, or sites that are influenced by other factors (e.g., horizontal strain, wind). However, the results highlight the limitations of constructing a model empirically. 3 Next, we develop a model that modifies a relationship from previous work to estimate the densification rate through viscosity and the evolution of microstructures. We define microstructural evolution by using micro-CT data from USP50 near South Pole, and run our model for USP50 as well as several other sites. Our results show good agreement; however, more work is necessary to further develop this model, including the collection of more microstructure data. Nevertheless, our research provides a key step towards producing a firn- densification model that estimates firn properties on the microscale and that can potentially be used in a range of climatic conditions and during climate transients. | |
| dc.embargo.terms | Open Access | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.other | Horlings_washington_0250O_21076.pdf | |
| dc.identifier.uri | http://hdl.handle.net/1773/45031 | |
| dc.language.iso | en_US | |
| dc.rights | none | |
| dc.subject | Firn | |
| dc.subject | Firn-densification model | |
| dc.subject | micro-CT data | |
| dc.subject | microstructures | |
| dc.subject | Geophysics | |
| dc.subject.other | Earth and space sciences | |
| dc.title | Modeling firn densification through viscosity and microstructures | |
| dc.type | Thesis |
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