1 INTRODUCTION  
2 GALAXY CLUSTER INFORMATION  
2.1 The WEAVE Wide-Field Cluster Survey  
2.2 The Three Hundred galaxy cluster simulations  
3 GENERATION OF MOCK OBSERVATIONS  
3.1 Optimizing the WWFCS field positions  
3.2 Deriving WWFCS cluster properties  
3.3 Generating the simulated cluster and galaxy samples  
3.4 Allocating spectroscopic fibres to mock galaxies using Configure  
3.5 Cosmic web extraction method  
4 RESULTS AND DISCUSSION  
4.1 Recovery of cluster galaxies after Configure  
4.2 Filament network comparison metrics  
4.3 Quantifying the quality of the recovered filament networks  
5 SUMMARY AND CONCLUSIONS