Reconstruction of the High Resolution Phase in a Closed Loop Adaptive Optics System
From MaRDI portal
Publication:3296467
DOI10.1137/19M1258426zbMath1443.85003OpenAlexW3022428247MaRDI QIDQ3296467
No author found.
Publication date: 7 July 2020
Published in: SIAM Journal on Imaging Sciences (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1137/19m1258426
Image analysis in multivariate analysis (62H35) Applications of statistics to physics (62P35) Planetary atmospheres (85A20) Computational methods for problems pertaining to astronomy and astrophysics (85-08) General questions in astronomy and astrophysics (85A04)
Related Items (1)
Cites Work
- Unnamed Item
- Distributed Optimization and Statistical Learning via the Alternating Direction Method of Multipliers
- A phase model for point spread function estimation in ground-based astronomy
- Cumulative wavefront reconstructor for the Shack-Hartmann sensor
- A framelet algorithm for enhancing video stills
- Optical Flow
- A new cumulative wavefront reconstructor for the Shack–Hartmann sensor
- Wavelet methods in multi-conjugate adaptive optics
- Iterative Wavefront Reconstruction for Astronomical Imaging
- Towards analytical model optimization in atmospheric tomography
- Inverse problems in astronomical adaptive optics
- On Optical Flow Models for Variational Motion Estimation
- Local All-Pass Geometric Deformations
- A new temporal control approach for SCAO systems
This page was built for publication: Reconstruction of the High Resolution Phase in a Closed Loop Adaptive Optics System
