Meta-optic Spectropolarimeter For Heliophysics Imaging
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Nanohmics and the City University of New York are developing a low-SWaP imaging spectropolarimeter for NASA heliophysics missions under solicitation NASA-SBIR-185433. The project utilizes a microfabricated multifunction meta-optic and a commercial off-the-shelf focal plane array to simultaneously collect polarization, spectral, and one-dimensional imaging data at video rates. This technology aims to reduce the mass and volume of existing spectropolarimeters to approximately one tenth of their current size while eliminating moving parts. The initial focus is on the H-alpha line at 656 nm to study the solar chromosphere and flare kernels, with future expansions planned for other visible and ultraviolet bands. The project is structured in two phases, moving from a brassboard demonstration at TRL 4 in Phase I to a ruggedized prototype at TRL 5 in Phase II. The sensor is designed for integration into SWaP-constrained vehicles such as CubeSats. Beyond heliophysics, the use of standard CMOS microfabrication allows for cost-effective commercialization across various sectors, including defense, security, and industrial monitoring. The effort is managed by the NASA SBIR/STTR Program and is designated as a total small business set-aside.
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TX, USASet-Aside
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Benefits: By providing imaging, polarimetry, and spectroscopy in a compact low-cost package, the proposed sensor is ideal for measurements on heliophysics missions – initially in red wavelengths to investigate H-alpha, but extensible to cover other VIS spectral bands. Combining polarization and spectral data will enable detailed investigation of regions of the chromosphere, including imaging across flare origin and reconnection spots along the solar limb. Inspiration for this project is to improve upon measurements from the solar Zurich IMaging POLarimeter (ZIMPOL) instrument, which measured spectrum and polarization across VIS bands of the solar spectrum, viewing the solar limb. With the addition of positional imaging, the spectropolarimeter will provide an understanding of the chromosphere’s polarization features, particularly solar flare kernels. Spectropolarimeter operation centered on the H-alpha line (656 nm) is a first step toward other VIS sub-bands, given its prominence in astrophysics as a consistent emission line across stars and gas clouds; a strong and reliable indicator. Subsequent advances through VIS will enable further spectropolarimetric studies of particle acceleration processes. The spectropolarimeter can also advance into the ultraviolet (UV) to study the K-corona layer and the Lyman-alpha band, to better understand magnetic field topography and reconnection points. Longer term, the team proposes integration of the multi-band imaging spectropolarimeter and multifunction meta-optic technologies into a range of instruments for NASA heliophysics missions, including CubeSats and other SWaP-constrained vehicle payloads. The advanced capabilities and low SWaP of meta-optics sensors will make them valuable for many applications in the petroleum, chemical, pharmaceutical, electric power, and microelectronics sectors. These commercial applications may include defense; security; vehicle autonomy; agriculture; food processing, oceanography; water resource monitoring; waste management, water treatment; monitoring of terrestrial sources of industrial gas emissions; emissions compliance control for refineries and factories; and intelligence, surveillance, and reconnaissance (ISR) for the Department of Defense (DoD) and Homeland Security (DHS). Low-cost, low-SWaP spectropolarimeters can be installed throughout these facilities and/or carried by UASs or SmallSats to collect data that can be used to increase safety, efficiency, and environmental compliance. Nanohmics intends to aggressively commercialize the low-SWaP spectropolarimeter and its component multifunction meta-optic technology, as it has done with other optical and imaging innovations. The single meta-optic, microfabricated using standard CMOS processes, performs the function of multiple conventional optical elements, reducing complexity and production cost while increasing robustness and space-readiness.
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