CAREER: A Portable Solar Adaptive Optics System for High-Resolution Imaging Investigations

The University Corporation, Northridge, Northridge CA

Investigators

Abstract

The PI will develop the first portable solar adaptive optics system (PSAO) at California State University Northridge (CSUN) for scientific observations in the 1 ìm to 4.5 ìm infrared band. He will use the PSAO to perform high-resolution solar imaging with the National Solar Observatory (NSO) 1.5-meter McMath-Pierce telescope (McMP) on Kitt Peak near Tucson, Arizona. The PSAO will take full advantage of the McMP's large aperture and high magnetic sensitivity in the IR. The PSAO will utilize a wave-front sensor and deformable mirror with 120 efficient actuators to efficiently correct for atmospheric turbulence, in order to provide high angular resolution images in the near IR. The expected scientific results will enhance our understanding of the dynamics and structure of small scale magnetic fields on the Sun. The PI also plans to explore and evaluate Multi-Conjugate Adaptive Optics (MCAO) approaches for solar imaging, since this technique provides a large corrected field of view for observing solar active regions. For nighttime astronomy MCAO systems, 3D tomographic wave-front sensing and reconstruction have been difficult problems to solve, since multiple laser guide stars are needed. The Sun, however, provides an excellent opportunity for MCAO tomographic wave-front sensing, since any number of equivalent 'guide stars' can be obtained from sites on the solar disk itself. The PI will use the PSAO's wave-front sensor to measure and reconstruct turbulence-induced wave-front errors at different altitudes, allowing a quantitative performance evaluation of the MCAO technique. Once the PSAO is fully demonstrated, the PI plans to transfer his techniques to the NSO at Kitt Peak and make 50% of PSAO observing time available to the wider solar community. His tomographic wave-front sensing and reconstruction efforts will be important steps forward in developing future solar MCAO technologies for solar telescopes. This project will also integrate research and education through the development of a new Laboratory for High-Resolution Solar Imaging at CSUN. This lab will be used intensively for teaching, training, and technology development at CSUN, and initially involve at least ten undergraduates, three graduate students, and one postdoctoral researcher. This project will provide long-term cross-disciplinary training in physics and astronomy to CSUN students, and the research results will be incorporated into courses taught by the PI. The proposed program will also create a long-term partnership between CSUN and the NSO, which will provide excellent opportunities for additional student training and education at Kitt Peak.