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Details

Autor(en) / Beteiligte
Titel
Micro-laminated pin array solar receivers for high flux heating of supercritical carbon dioxide part 1: Design and fabrication methods
Ist Teil von
  • Solar energy, 2024-05, Vol.273 (C), p.112403, Article 112403
Ort / Verlag
United States: Elsevier Ltd
Erscheinungsjahr
2024
Quelle
Alma/SFX Local Collection
Beschreibungen/Notizen
  • •High temperature solar receiver design and fabrication methods.•Evaluation of diffusion bonding, brazing, and welding methods.•Development of separate and combined effects testing.•Prototype fabrication and high-pressure testing. Development of gas-based solar receivers that can withstand the extreme temperatures (>700 °C) and high pressures required in next generation concentrating solar plants remains a significant challenge. This study presents an investigation of the design and fabrication methods of a prototype modular, micro-pin solar receiver for directly heating supercritical carbon dioxide from temperatures of 550 °C to 720 °C at a pressure of 20 MPa and an incident flux > 100 W cm−2. The receiver is fabricated from high nickel content Haynes 230 alloy. Multiple failure modes related to design and fabrication methods were identified in a first-generation prototype. Here, these failure modes are mitigated by the introduction of improved diffusion bonding, brazing, design of the receiver header and micro-pin array. The efficacy of each improvement was evaluated separately using a combination of simulations and lab-scale experiments. The design improvements were then integrated into sub-scale (5 cm × 5 cm) and prototype scale (15 cm × 15 cm) test devices. The study resulted in the successful fabrication and proof and cyclic pressure testing of a prototype receiver that was tested in a concentrating solar dish. The results of this study can guide the development process of other high temperature receiver technologies that must operate at extreme pressures and incident fluxes.
Sprache
Englisch
Identifikatoren
ISSN: 0038-092X
eISSN: 1471-1257
DOI: 10.1016/j.solener.2024.112403
Titel-ID: cdi_osti_scitechconnect_2336815

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