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Prototype Modification for Prototype Isolation and Detection Optimization

Discuss modifications for optimizing detectors, isolating parts, addressing dead zones, accommodating telescope gaps, and enhancing solid angle detection. Consider electronics board separation and thermal calculations for efficient performance.

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Prototype Modification for Prototype Isolation and Detection Optimization

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  1. DESIGN Points to discuss

  2. MODIFICATION of the PROTOTYPES (LNL/GANIL) Isolating part (16)

  3. Overall detection solid angle Taking into account Gap between telescopes Dead zones around Si 0.6mm ~86% 22*22 ~90% 44*44

  4. TELESCOPES arrangement C2 C3 C1 Gap between Telescopes C4B C4A

  5. Possible mounting 40*40 Forward Si Backward Si Bonding Dead Zone Tunnel 0.5 Flexible Kapton

  6. 1m long Preamplifiers Question:Could we separate the electronics board?

  7. SPECIFICATIONS Physics specifications ? WG2 Dimensions telescopes ? WG7 Electronics board Specifications ? WG3 Bonding wires on 0.5mm section ? WG5

  8. OVERALL ELECTRONICS BOARDS

  9. BASIC BLOCK Cooling ring Backwards dismantling SUGGESTION: Make a complete basic block

  10. THERMAL CALCULATION Aluminium λ=120W/m.K Cu λ=400 W/m.K Heat Convection 15°C Epoxy FR4 λ=0.3 W/m.K Thermal load on the 2 faces of each electronics board.(Simulation of the Aluminium drain)

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