Wavelength Shifters for Water Cherenkov Detectors

The light yield of a water-based Cherenkov detector can be significantly improved by adding a wavelength shifter. Wavelength shifter (WLS) molecules absorb ultraviolet photons and re-emit them at longer wavelengths where typical photomultiplier tubes are more sensitive. In this study, several wavelength shifter compounds are tested for possible deployment in the Sudbury Neutrino Observatory (SNO). Test results on optical properties and chemical compatibility for a few WLS candidates are reported; together with timing and gain measurements. A Monte Carlo simulation of the SNO detector response is used to estimate the total light gain with WLS. Finally, a cosmic ray Cherenkov detector was built to investigate the optical properties of WLS.Comment: 13 pages, 3 figure

UCI Rocket Project

Abstract: The UCI Rocket Project is an undergraduate student team pushing the boundaries of collegiate rocketry through the design and fabrication of liquid-fueled rockets. Our project provides engineering students with the opportunity to work on complex systems within a multidisciplinary team. The systems are designed using professional modeling and simulation software, innovative manufacturing and fabrication solutions, and strict validation procedures. Project Advisor: Professor Mark Walte

UCI Rocket Project

Abstract: The UCI Rocket Project is an undergraduate student team pushing the boundaries of collegiate rocketry through the design and fabrication of liquid-fueled rockets. Our project provides engineering students with the opportunity to work on complex systems within a multidisciplinary team. The systems are designed using professional modeling and simulation software, innovative manufacturing and fabrication solutions, and strict validation procedures. Project Advisor: Professor Mark Walte