PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
Knowledge of the refractive index structure constant profile at an astronomical site is crucial before developing a Multi-Conjugate Adaptive Optics (MCAO) system at that site. The S-DIMM+ (S-Differential Image Motion Monitor+) method proposed by Scharmer and van Werkhoven uses the images recorded by a SHWFS (ShackHartmann Wavefront Sensor) to estimate the profile. We have performed simulations of the same using simulated solar granulation images (which are the “objects”) and multiple layers of the atmosphere characterised by Kolmogorov turbulence, a telescope of given aperture and finally a SHWFS. The images formed using the SHWFS are then processed using an inversion code developed by us to get the turbulence strength profile. We found that the code was able to invert the data satisfactorily upto a height of 10 km with our system parameters.
Saraswathi Kalyani Subramanian andSridharan Rengaswamy
"Forward modelling of turbulence strength profile estimation using S-DIMM+", Proc. SPIE 12638, Women in Optics and Photonics in India 2022, 1263812 (11 May 2023); https://doi.org/10.1117/12.2671735
ACCESS THE FULL ARTICLE
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Saraswathi Kalyani Subramanian, Sridharan Rengaswamy, "Forward modelling of turbulence strength profile estimation using S-DIMM+," Proc. SPIE 12638, Women in Optics and Photonics in India 2022, 1263812 (11 May 2023); https://doi.org/10.1117/12.2671735