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Table 1.

Description of variables.

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Table 1 Expand

Fig 1.

Desert locust dual phase population dynamics schematic diagram.

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Fig 1 Expand

Fig 2.

Profile of temperature-dependent oviposition rate of adult desert locusts using the function (7).

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Fig 3.

Profile of temperature-dependent desert locust egg hatching rate (1/days).

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Fig 3 Expand

Fig 4.

Profile of egg mortality rate of desert locusts as a function of soil temperature (°C).

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Fig 4 Expand

Fig 5.

Profile of the relationship between air temperature (°C) versus desert locust hopper development rate (1/day).

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Fig 5 Expand

Fig 6.

Profile of solitarious and gregarious nymphal mortality rate as a function of air temperature.

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Fig 6 Expand

Fig 7.

Profile of solitarious and gregarious temperature dependent adult mortality.

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Fig 7 Expand

Fig 8.

Partial rank correlation coefficients (PRCCs) between model parameters and the basic offspring number ().

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Fig 8 Expand

Table 2.

Description of parameters.

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Table 2 Expand

Fig 9.

Time series of desert locust population densities for different initial conditions converging towards the extinction equilibrium.

The autonomous model (14) was used with parameters from Table 2 with ϕ = 1.75, resulting in a basic offspring number .

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Fig 9 Expand

Fig 10.

Time series of desert locust population densities (eggs, hoppers, bands, solitaries, and gregarious adults) converging towards the non-trivial equilibrium.

The autonomous model (14) was used with parameters from Table 2 and ϕ = 25, μh = 0.25, μb = 0.3, resulting in a basic offspring number . Various initial conditions were utilized to illustrate the stability of the equilibrium.

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Fig 10 Expand

Fig 11.

A simulation examining the effects of temperature-dependent fecundity rates(ϕ(T)) on the system (4).

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Fig 11 Expand

Fig 12.

Simulated impact of temperature-dependent egg hatching rate σ(T) on desert locust population dynamics (4).

Model parameters based on Table 2 with ω = 2, T0 = 20°C, T1 = 2°C, κ = 100.

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Fig 12 Expand

Fig 13.

The impact of γh(T).

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Fig 14.

The impact of γb(T).

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Fig 14 Expand