The mixing and atomization of propellants is often characterized by optically dense flow fields and complex breakup dynamics. In the development of propulsion systems, the complexity of relevant physics and the range of spatio-temporal scales often makes computational simulation impractical for full scale injector elements; consequently, continued research into improved systems for experimental flow diagnostics is ongoing. One area of non-invasive flow diagnostics which has seen widespread growth is using synchrotron based x-ray diagostics. Over the past 3 years, a series of water and cryogenic based experiments were performed at the Advanced Photon Source, Argonne National Lab, on a NASA in-house designed swirl co-axial rocket injector, designed for operation using liquid oxygen and liquid methane in support of Project Morpheus. A range of techniques, such as x-ray fluorescence and time-averaged radiography were performed providing qualitative and quantitative mass and phase distributions, and were complemented by investigations using time-resolved radiography and white beam imaging, which provided information on breakup and mixing dynamics. Results of these investigations are presented, and conclusions regarding the viability of x-ray based diagnostics are discussed.
I. Nomenclature d= diameter of pressure swirl atomizer, m D = diameter of gas annulus, m I = x-ray signal intensity, photons/s I 0 = x-ray source intensity, photons/ṡ m = mass flow rate, kg/s V = gas phase velocity, m/s Re g = gas phase Reynolds number ν = gas phase kinematic viscosity, kg/m · s ρ = gas phase density,kg/m 3 Subscripts g = gas i = inner diameter o = outer diameter