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Proceedings Article

AO-308: the high-order adaptive optics system at Big Bear Solar Observatory

[+] Author Affiliations
Sergey Shumko, Nicolas Gorceix, Seonghwan Choi, Aglaé Kellerer, Wenda Cao, Volodymyr Abramenko

Big Bear Solar Observatory (United States)

Philip R. Goode

New Jersey Institute of Technology (United States)

Kit Richards, Thomas R. Rimmele, Jose Marino

National Solar Observatory (United States)

Proc. SPIE 9148, Adaptive Optics Systems IV, 914835 (August 7, 2014); doi:10.1117/12.2056731
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From Conference Volume 9148

  • Adaptive Optics Systems IV
  • Enrico Marchetti; Laird M. Close; Jean-Pierre Véran
  • Montréal, Quebec, Canada | June 22, 2014

abstract

In this paper we present Big Bear Solar Observatory’s (BBSO) newest adaptive optics system – AO-308. AO-308 is a result of collaboration between BBSO and National Solar Observatory (NSO). AO-308 uses a 357 actuators deformable mirror (DM) from Xinetics and its wave front sensor (WFS) has 308 sub-apertures. The WFS uses a Phantom V7.3 camera which runs at 2000 Hz with the region of interest of 416×400 pixels. AO-308 utilizes digital signal processors (DSPs) for image processing. AO-308 has been successfully used during the 2013 observing season. The system can correct up to 310 modes providing diffraction limited images at all wavelengths of interest. © (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Citation

Sergey Shumko ; Nicolas Gorceix ; Seonghwan Choi ; Aglaé Kellerer ; Wenda Cao, et al.
" AO-308: the high-order adaptive optics system at Big Bear Solar Observatory ", Proc. SPIE 9148, Adaptive Optics Systems IV, 914835 (August 7, 2014); doi:10.1117/12.2056731; http://dx.doi.org/10.1117/12.2056731


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