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EUV Photon Sieves for Milli-Arcsecond Imaging of the Solar Corona

Completed TRL 3 (started at 3, targeting 4)

Description

A photon sieve is a variant of a Fresnel zone plate that can achieve diffraction-limited angular resolution in the extreme ultraviolet (EUV). Existing EUV instruments such as SDO/AIA and Hi-C are reflecting telescopes, and fall short by an order of magnitude or more from achieving the diffraction limit, because the mirrors cannot be figured to the requisite accuracy. Photon sieves offer the ability to obtain diffraction-limited EUV images using imaging elements with greatly relaxed manufacturing tolerances: sub-micron as opposed to the sub-nanometer requirements for conventional telescopes. Furthermore, sieves can isolate strong EUV emission lines for a wide range of temperatures in the solar atmosphere, including eruptive events. The unprecedented resolution achieved will allow us to observe individual dissipation regions in the solar corona and at last understand how the corona is powered. Understanding the heating of coronal plasmas and solar eruptive events are at the heart of NASA's strategic goal to Understand the Sun and its interactions with Earth and the solar system. Therefore, we propose to manufacture large-aperture photon sieves, demonstrate diffraction-limited EUV imaging in the laboratory, and perform environmental testing of the sieves for space flight.

Benefits

Support NASA's Heliophysics strategic science objectives to understand the Sun and its interactions with Earth and the solar system, including space weather. This will be achieved by developing/demonstrating instrumentation technology necessary to address the following science goals: Explore the physical processes in the space environment from the Sun to the Earth and throughout the solar system; Advance our understanding of the connections that link the Sun, the Earth, planetary space environments, and the outer reaches of our solar system; Develop the knowledge and capability to detect and predict extreme conditions in space to protect life and society and to safeguard human and robotic explorers beyond Earth.

Details

Technology areaSensors and Instruments > Observatories > Distributed Aperture
ProgramHeliophysics Technology and Instrument Development for Science (H-TIDeS)
Lead organizationGoddard Space Flight Center, Greenbelt, MD
Start date2018-02-01
End date2023-12-01

Project contacts

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This is early/mid-stage (TRL 3) — the most realistic path in is NASA SBIR/STTR, which funds small businesses and research institutions to develop technology aligned with NASA's needs (equity-free, phased funding). Check whether a current SBIR/STTR solicitation topic overlaps with this project's technology area, or contact the project directly (above) to ask.

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