Input data to the model must be prepared in a GIS such as ESRI's ArcGIS or MapInfo. This base data is then converted into a format read by PHOENIX which is an ASCII grid broken into data tiles. Tiling can be achieved manually, but is better achieved using ancillary support tools provided as part of PHOENIX, installed as part of the ArcGIS Toolbox.

In some cases an Input to the model is produced by taking several data files provided to PHOENIX (as configuration or spatial data sets) and performing some pre-processing. The relationship between inputs and file names used by PHOENIX as described in Appendix 2. For detailed instructions on preparing data for PHOENIX (including descriptions of preparing individual input layers), please refer to the PHOENIX Input Data Guide.

Generally, PHOENIX input data has the following requirements:

All data layers must be in the same coordinate system, and this must be a map grid projection (grid reference in metres) not a geographic one (latitude and longitude in degrees). In Victoria, using 'VicGrid 94' is recommended, which is a Lambert Conformal Conic Projection with a GDA 94 reference Datum. Across Australia, using 'Geoscience Australia Lambert 94' projection is recommended, which is also a Lambert Conformal Conic Projection with a GDA 94 reference Datum.
The only data layer that must be provided is fuel types. However, other layers are required for realistic simulations. If there is no fuel types file location specified, then the input value defaults to zero (no fuel, or bare area).
As all data layers must be in the same coordinate system only one GIS spatial projection file is required.
Layers are broken into 'tiles' and packaged as zip files, to decrease the size and number of files that have to be copied and transported. The zipped files are unzipped on the first run of a simulation session.

4.1 Fuel types

4.1.1 Purpose

Fuel types is a mandatory input layer required by PHOENIX to generate fine fuel levels for each fuel stratum (surface, elevated and bark – see Hines et al. 2010 for details).

4.1.2 Basis

Fuel type is built upon spatial vegetation type data.

In Victoria, 900 or so vegetation types (EVCs) were manually assigned to one of about 40 fuel types by Kevin Tolhurst on the basis of his knowledge and experience. This was initially done to enable a proof-of-concept run of the PHOENIX simulation. However, this initial classification is largely still being used. In some areas, there have been efforts to improve/correct this classification. In NSW, a significant effort was made to map the fuel types and their accumulation rates after fire, as part of a separate research program. South Australia, Western Australia, Tasmania and Queensland have undertaken similar processes to what has occurred in Victoria.

4.1.3 Assumptions and limitations

Vegetation type is used because it is assumed that vegetation type is the most likely layer to be kept up-to-date by government agencies. The mapping must cover the whole area. Areas with no fuel type mapped will be assumed to not carry fire.

Fuel types with no elevated or bark fuel are assumed to be grasslands.

4.1.4 User interactions

Due to varying vegetation classification standards in different jurisdictions, vegetation types must be converted/aggregated to fuel types by the user. The user prepares the input layer by assigning each vegetation type to a user-defined fuel type for use in PHOENIX. The maximum fine fuel levels for each fuel stratum (surface, elevated and bark) and the rate of reaccumulation in each stratum after burning must be specified for each fuel type defined.

4.1.5 Description

Management agencies commonly spatially classify landscapes into distinct vegetation types suitable for use in modelling (Sun et al. 1998). It is acknowledged that there are several vegetation type classifications and a range of mapping detail and quality within some states and between states. Therefore, in the creation of the PHOENIX fuel layer, each vegetation type must be classified into a fuel type and assigned an integer code ('FuelCode') by the user. An example of a fuel type classification is shown in Table 3. The fuel mapping must cover the whole area being simulated. Areas with no fuel type mapped will be assumed to carry no fuel (e.g. a water body) and therefore will not carry fire.
A lookup table of fine fuel parameters must then be defined and conform to the PHOENIX convention. This lookup table is typically called 'Fueltype.xml' and joins to the fuel type layer via the FuelCode. Section 5.7: Fuel Accumulation has more information.

Fine fuel hazard levels are converted to an equivalent fine fuel load (t/ha). While coarser fuels are consumed during a fire, the combustion of fine fuels is the process that predominantly determines spread rates. Fuels are considered as three separate strata; surface (which includes near-surface fuels), elevated fuel and bark, in accordance with forest fuel measurement standards in Southern Australia (McCarthy et al. 1999; Hines et al. 2010). Fuel classes that have no elevated or bark fuels are considered by PHOENIX as grasslands and are processed using functions derived from the CSIRO grassland fire spread model (Cheney et al. 1998).

Table 3. PHOENIX fuel types currently recognised in southern Australia.

Veg Type	Code	FuelCode	Description	Fuel Characteristics
Forest	F01	15	Rainforest	dense vegetation with little dead material, epiphytes, vines, ferns, rarely dry
	F02	32	Wet Forest with rainforest understory	wet sclerophyll forest with a mesic understorey
	F03	13	Riparian Forest shrub	dense vegetation but with a small proportion of dead material
	F04	11	Wet Forest shrub & wiregrass	high biomass forest, but with little dead suspended material unless wiregrass present
	F05	12	Damp Forest shrub	dense understorey and potentially high bark hazard (karri)
	F06	40	Semi-mesic Sclerophyll forest	forest with semi-mesic shrubs and flammable grasses, sedge understorey
	F07	33	Swamp Forest	dense Melaleuca forest with little understorey
	F08	6	Forest with shrub	potentially high bark hazard, shrubs moderate flammability (mixed jarrah/karri)
	F09	7	Forest herb-rich	potentially high bark hazard, little elevated fuel
	F10	45	Dry Forest shrubs	dry forest with continuous understorey, (southern jarrah)
	F11	8	Dry Open Forest shrub/herbs	dry forest with open understorey (northern jarrah)
Grass/sedges	G01	16	High Elevation Grassland	dense sward of tussock grasses or herbs, high cover
	G02	4	Moist Sedgeland / Grassland	dense sward, potentially high dead component, button grass
	G03	29	Ephemeral grass/sedge/herbs	dense grass and sedges with potentially high levels of dead suspended material
	G04	20	Temperate Grassland / Sedgeland	grasses and sedges widespread, but varying in biomass
	G05	44	Hummock grassland	hummock grassland, discontinuous surface fuels
Herbs	H01	30	Moorland / Feldmarks	low flammability cushion plants
	H02	36	Alpine herbland	dense, upright, low flammability herbs
	H03	34	Wet herbland	freshwater herbs on mud flats
	H03	37	Wet herbland	low herbs in seasonally inundated lakebeds or wetlands
Mallee	M01	27	Mallee chenopod	low flammability except after exceptional rain bringing grasses
	M02	42	Mallee grass	mallee woodland with predominantly grass understorey
	M03	25	Mallee shrub/heath	continuous shrub layer but amount of dead material depending on species present
	M04	26	Mallee spinifex	discontinuous fuels, very flammable under windy conditions
Bare	NIL	0	Water, sand, no vegetation	fuel absent
Plantations	P01	98	Softwood Plantation	dense canopy with continuous surface fuels
	P02	99	Hardwood Plantation	uniform canopy with continuous surface fuels
Shrubs	S01	17	High Elevation Shrubland/Heath	dense cover of shrubs with surface fuel largely under plants
	S02	14	Riparian shrubland	dense vegetation with little dead material
	S03	35	Wet Scrub	flammable shrubland with high level of dead elevated fuels
	S04	1	Moist Shrubland	dense shrubland, salt affected
	S05	31	Dry Closed Shrubland	tea-tree or paperbark thickets, little understorey
	S06	21	Broombush / Shrubland / Tea-tree	dense shrubland, but with relatively low level of dead material
	S07	10	Sparse shrubland	sparse shrubby vegetation with discontinuous surface fuels
	S08	3	Low flammable Shrubs	low flammability except after exceptional rain bringing grasses
	S09	38	Mangroves / Aquatic Herbs	trees, shrubs and herbs in permanent water, unburnable
Heaths	S10	23	Wet Heath	dense heath possibly with dense sedgy undergrowth
	S11	24	Dry Heath	dense heath with significant amounts of dead material
Woodland	W01	18	High Elevation Woodland shrub	wooded area with shrubby understorey
	W02	19	High Elevation Woodland grass	wooded area with continuous grass tussocks
	W03	97	Orchard / Vineyard	orchard or vineyard
	W04	2	Moist Woodland	low trees, shrubby, sedgy understorey, bark hazard
	W05	22	Woodland bracken/shrubby	wooded area with varying understorey, but not heathy
	W06	9	Woodland Grass/Herb-rich	surface fuels dominated by grass and herbs
	W07	5	Woodland Heath	flammable shrubs and high bark hazard
	W08	41	Gum Woodland heath/shrub	gum woodland with moderate bark hazard, heath/shrub understorey
	W09	43	Gum Woodland grass/herbs	gum woodland with moderate bark hazard, herbaceous understorey
	W10	39	Savanna grasslands	tall flammable grasses in an open woodland
	W11	28	Woodland Callitris/Belah	low flammability except after exceptional rain bringing grasses

4.2 Wind reduction factors

4.2.1 Purpose

Bureau of Meteorology forecast wind data is provided at 10 m above ground. PHOENIX takes this data and converts it to wind speeds at 1.5 m above ground for use by various PHOENIX models.

4.2.2 Basis

Wind reduction factors are specified by the user for each defined fuel type in the Fueltype.xml file (See Section 5.7: Fuel Accumulation).

4.2.3 Assumptions and limitations

It is assumed that the wind at 1.5 m is the 'mid-flame height' wind speed which is clearly untrue for very low-intensity fires and very high-intensity fires. It also assumes that the wind reduction factor is a constant, but it is known to vary from day to night and with the magnitude of the wind speed in the open.

4.2.4 User interactions

Wind reduction factors can only be changed by the user by redefining the fuel type characteristics in the Fueltype.xml file.

4.2.5 Description

Wind reduction factors are assigned to each fuel type in the fueltype.xml file. Values for the wind reduction factors are not well studied and so many will have to be estimated by an experienced fire behaviour scientist. Some guidance on the values of wind reduction factors can be gained from the Western Australian 'Red Book' (Sneeuwjagt and Peet 1998 p.30). The wind reduction factor is used to estimate the mid-flame height wind speed within the vegetation based on the observed or forecast wind speed measured at 10 m in the open. In 18 m high open eucalypt forest, McArthur assumed that the wind reduction factor at 1.5 m above the ground was a factor of 3. In Jarrah forest in Western Australia, Project Vesta found that the wind reduction factor at 5 m above the ground was also a factor of 3. In grassland, there is no wind reduction factor assumed so the value is set to 1. In grassy woodland in northern Australia, Cheney et al. (1998) found the wind reduction factor to be a factor of 2. Since flame height varies from low-intensity surface fires to high-intensity crown fires, the reality is that the wind reduction factor is not constant even for a single fuel type, but a single typical value is used. Work by Kangmin Moon (2016) developed a model of estimating the wind reduction factor in different fuel types at different heights which would enable the use of a dynamic wind reduction factor, but this has not yet been incorporated into PHOENIX.

The cell wind reduction factor is also used to estimate an approximate leaf area index (LAI) used to calculate shading based on Beer's law (Silberstein, Sivapalan et al. 2003). Refer to Section 5.6: Solar Radiation Model for further information on how shading is used.

4.3 Fire history

4.3.1 Purpose

Fuel types are used in conjunction with the fire history layer to generate fuel levels at the time of the simulation. Based on the time of ignition specified by the user, fuel levels are calculated through the combination of fuel type and the time since the last fire using fuel accumulation curves defined in the fuel type conversion file.

4.3.2 Basis

This layer is based upon fire history provided by the user.

4.3.3 Assumptions and limitations

In the case of overlapping fire histories, PHOENIX only uses the most recent fire occurrence.

4.3.4 User interactions

PHOENIX uses the fuel accumulation model (see Section 5.7: Fuel Accumulation) to calculate fine fuel hazard classes which are then converted to an equivalent fuel load (t/ha) for surface, elevated and bark fuels. The accumulation curves are part of the fuel type conversion file.

The user can upload a supplementary fire history layer to PHOENIX to capture recent fire events or to explore the effect of hypothetical fires in the landscape.

4.3.5 Description

Fuel types are used in conjunction with a user-provided fire history layer to create fuel layer information used in PHOENIX simulations and stored in the Fire Grid. The time since the most recent fire is used to estimate fuel levels using negative exponential accumulation curves (discussed in Section 5.7: Fuel Accumulation). As data is retained for only the most recent fires (see Figure 9), where historic fires are being simulated, the fire history layer must be adjusted to be representative of the appropriate conditions.

Figure 9. Diagram of how PHOENIX treats overlapping fire history. On the left, two fires have been mapped, one in 1972 and the other in 1985. On the right, a new fire in 2008 has overlapped these earlier fires and has replaced their fire history in the overlapping areas.

ESRI Shapefiles can be used to supplement the baseline fire history layer for particular simulation runs. This provision is made to account for fires that have occurred since the baseline fire history was processed or to enable hypothetical prescribed burning scenarios to be quickly evaluated. The supplementary fire history is added to any existing fire history layer and processed in the same manner as the fire history stored in the Fire Grid.

TRG Chapter 4: Inputs

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