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M odel for a dune field (chapters 5 and 6)

1) Physical Basis: The sim ulation rules were not derived from fundam ental equa­ tions, b u t introduced phenomenologically, based on observations and aerody­ nam ic considerations. For example, if wind blows in a desert, sand is tran sp o rted in th e wind direction. The stronger th e wind, the greater distance sand is trans­ ported. These form the physical background of the slab tra n sp o rt in th e model. A nother exam ple is th a t avalanching occurs in n a tu re if th e angle of a sandy slope exceeds th e angle of repose of ab ou t 32°. In th e m odel avalanching dynam ­ ics has been introduced in th e same m anner, w ithout discussing its microscopic origin, hence th e phenomenological basis of the model. O th er dynam ics such as wind speedup, slab bouncing and th e shadow zone have also been introduced phenomenologically, though the origins of all these processes can be discussed in some detail.

2) Simplicity: T he sim ulation rules are simple. T his is evident when comparing to models w ith th e Navier-Stokes equation, where in teractin g air pressure and three com ponents of wind velocity are defined on a three-dim ensional continuous space { x ,y ,z ) . Consequently, th e com putational burden for such conventional models is very heavy. In the present model on th e oth er hand, slab tran sp o rt length (L) is defined on a two-dimensional discrete space, and tra n sp o rt length is simply a function of local num ber of slabs at a location.

3) G enerality and Richness: It has already been shown th a t a lattice model can be effective for vegetated dune fields (de C astro, 1995) (section 2.7.2). The present study has assum ed a fiat hard surface, on which slabs are piled up. By creating undulations on th is hard surface, the effects of existing topography could be sim­ ulated. Sim ulations are expected to reproduce, for exam ple, climbing and falling dunes (Lancaster, 1995, pp82-83) (generality). The m odel has been shown to mimic some of a variety of dune p attern s (dome, barchan, transverse, linear and star-like dunes), and to enable system atic understanding of m any different envi­ ronm ents, according to wind environm ent (strength and directional complexity)

and sand availability (richness).

4) P o ten tial for Scaling Up and Down: The model m ay apply to an inhomoge- neous dune field by introducing regionally different p aram eters {i.e. a distributed model), if m ore com putational capacity were to be available (scaling up). The use of discrete dynam ics has already been recognised to be effective in th e study of ripples (N ishim ori and Ouchi, 1993; Anderson and B unas, 1993; Landry and W erner, 1994) (section 2.7.2) (scaling down).

In short, b o th m odels are generally satisfactory in th e light of these four criteria. Still, th e first m odel suffers lack of richness, in th a t it cannot go beyond two- dim ensional, equilibrium bedforms. The physical basis of th e second model is still not secure. However, by sim ulating m any other types of dune {i.e. collecting more circum stantial evidence), th e model may become more convincing.

7.2.3

E ngineering asp ects

In respect of engineering, th e m ost notable success is th e estim ation of dune mi­ gration speed. Civil engineers will benefit from the first m odel when exploiting deserts w ith roads or pipelines for oil and gas. The ability to predict responses in shape and m igration speed to environm ental change is im p o rtan t. More specifi­ cally, it is im p o rta n t to investigate th e dynamics of dunes under rare high winds. Engineers are th o u g h t to be interested in how dunes th a t have been developed in m odest w ind conditions change in shape and in m igration speed during a storm, which is a sh o rt-term event of a day or a few days. In such conditions, the as­ sum ption of equilibrium is clearly inappropriate, and th e dune field model may be able to take over th e predictive role from the kinem atic model. In th e dune field model, as b o th sp atial and tem poral scales can be estim ated, a storm event of a certain d u ratio n can easily be sim ulated. In th e ‘sto rm ’, th e slab tran sp o rt length is increased for a certain period of tim e such th a t sand flux in th e model conforms to th e n a tu ra l behaviour a t a considered w ind speed (section 6.3.2).

Also using th e dune field model, effects of pre-existing topography such as rocks on dune dynam ics can be investigated.

7.2.4

C ontributions to geom orphology in general and to