Coded Aperture Imaging: novel approaches to high-energy high-resolution laboratory imaging

Rapid advancement is being made in laser driven x-ray and particle sources, pushing the boundaries in temporal duration, spatial and spectral distribution, and maximum energy. These advancements need to be complimented with development of imaging capabilities, in order to fully characterise and utilise the new source potential. Here, coded apertures are used to investigate novel approaches to high-energy high-resolution aperture based imaging. Firstly, coded aperture theory is applied to high-energy x-ray sources such as those generated using laser wakefield techniques. The coded aperture is compared to a single pinhole aperture, to discuss whether the prior assumption of highly attenuating substrates is required when using coded apertures. The coded aperture with scatter and partial attenuation included, dubbed a `CASPA', is demonstrated with a 511 keV source simulation, showing that the fully attenuating 18~mm thick tungsten substrate for a single pinhole can be replaced with a 250 um thick tungsten CASPA. Furthermore, the thin CASPA is not mechanism specific, and the physical processes behind the scatter and partial attenuation is found to be inconsequential as long as the combined result yields adequate hologram contrast for image decoding to occur. Secondly, an investigation is conducted into imaging with spectral and spatial information for applications such as laser-solid interaction hotspots. Combing coded apertures with Ross pair filters, a banded spectrally-resolving coded aperture is discussed, dubbed a `BaSCA', using multiple non-redundant array designs on a single aperture and single non-spectrally resolving detector. Finally, the application of a CASPA for imaging high-resolution high-energy neutron sources from inertial confinement fusion experiments is discussed. Using the National Ignition Facility at Lawrence Livermore National Laboratory as an example, a CASPA is designed for the 14.1 MeV neutrons, and reconstruction techniques discussed. In comparison to the currently implemented 20 cm thick gold grand array, it is suggested here that a 10 mm tungsten CASPA would suffice - potentially reducing manufacturing costs, increasing ease of implementation and field of view.