Key research themes
1. How can super-resolution techniques improve spatial frequency reconstruction in adaptive optics wavefront sensing?
This research area focuses on advancing wavefront reconstruction by surpassing the classical Nyquist-Shannon limit through super-resolution (SR) techniques. Particularly relevant in adaptive optics (AO) for astronomical instruments and extremely large telescopes (ELTs), SR approaches aim to enhance the spatial resolution of wavefront measurements by combining multiple low-resolution wavefront sensor (WFS) samples, exploiting both statistical regularization and geometric sample diversity. This theme matters because it addresses the fundamental limitation on wavefront reconstruction accuracy set by sensor resolution and noise, directly impacting the imaging performance of AO systems in astronomy.
2. What numerical and modal reconstruction methods enable accurate wavefront estimation from slope measurements over general and evolving apertures?
Wavefront estimation from gradient-based sensors like Shack-Hartmann commonly requires robust numerical methods to reconstruct the wavefront phase from local slope data. This theme investigates advances in modal approaches, notably numerical orthogonal transformation and orthogonal polynomial bases adapted for arbitrary and dynamically varying apertures. Such work is critical for applications requiring non-circular apertures or where the pupil shape evolves (e.g. scanning sensors), ensuring precise wavefront estimation essential for AO correction and optical testing.
3. How can innovative wavefront sensing designs and sensors overcome dynamic range and wavelength limitations inherent to traditional Shack-Hartmann sensors?
This research area addresses the intrinsic constraints of classical Shack-Hartmann wavefront sensors (SHWFS), primarily limited dynamic range imposed by microlens detection areas and wavelength dependency affecting sensor performance. It encompasses novel sensor concepts using holography, coded phase masks, and common-path interferometry to expand sensitivity, dynamic range, and spectral coverage, crucial for applications from astronomical AO to exoplanet imaging and high-contrast systems.