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

Sergey Shumko; Nicolas Gorceix; Seonghwan Choi; Aglaé Kellerer; Wenda Cao; Philip R. Goode; Volodymyr Abramenko; Kit Richards; Thomas R. Rimmele; Jose Marino

doi:10.1117/12.2056731

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

Sergey Shumko, Nicolas Gorceix, Seonghwan Choi, Aglaé Kellerer, Wenda Cao, Philip R. Goode, Volodymyr Abramenko, Kit Richards, Thomas R. Rimmele, Jose Marino

Center For Solar Terrestrial Research - Big Bear Solar Observatory

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

35 Scopus citations

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.

Original language	English (US)
Title of host publication	Adaptive Optics Systems IV
Editors	Jean-Pierre Veran, Enrico Marchetti, Laird M. Close
Publisher	SPIE
ISBN (Electronic)	9780819496164
DOIs	https://doi.org/10.1117/12.2056731
State	Published - 2014
Event	Adaptive Optics Systems IV - Montreal, Canada Duration: Jun 22 2014 → Jun 27 2014

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9148
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Adaptive Optics Systems IV
Country/Territory	Canada
City	Montreal
Period	6/22/14 → 6/27/14

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Keywords

AO-308
DSP
NST
adaptive optics

Access to Document

10.1117/12.2056731

Cite this

Shumko, S., Gorceix, N., Choi, S., Kellerer, A., Cao, W., Goode, P. R., Abramenko, V., Richards, K., Rimmele, T. R., & Marino, J. (2014). AO-308: The high-order adaptive optics system at Big Bear Solar Observatory. In J.-P. Veran, E. Marchetti, & L. M. Close (Eds.), Adaptive Optics Systems IV Article 914835 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9148). SPIE. https://doi.org/10.1117/12.2056731

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title = "AO-308: The high-order adaptive optics system at Big Bear Solar Observatory",

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.",

keywords = "AO-308, DSP, NST, adaptive optics",

author = "Sergey Shumko and Nicolas Gorceix and Seonghwan Choi and Agla{\'e} Kellerer and Wenda Cao and Goode, {Philip R.} and Volodymyr Abramenko and Kit Richards and Rimmele, {Thomas R.} and Jose Marino",

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year = "2014",

doi = "10.1117/12.2056731",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Jean-Pierre Veran and Enrico Marchetti and Close, {Laird M.}",

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Shumko, S, Gorceix, N, Choi, S, Kellerer, A, Cao, W, Goode, PR, Abramenko, V, Richards, K, Rimmele, TR & Marino, J 2014, AO-308: The high-order adaptive optics system at Big Bear Solar Observatory. in J-P Veran, E Marchetti & LM Close (eds), Adaptive Optics Systems IV., 914835, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9148, SPIE, Adaptive Optics Systems IV, Montreal, Canada, 6/22/14. https://doi.org/10.1117/12.2056731

AO-308: The high-order adaptive optics system at Big Bear Solar Observatory. / Shumko, Sergey; Gorceix, Nicolas; Choi, Seonghwan et al.
Adaptive Optics Systems IV. ed. / Jean-Pierre Veran; Enrico Marchetti; Laird M. Close. SPIE, 2014. 914835 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9148).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - AO-308

T2 - Adaptive Optics Systems IV

AU - Shumko, Sergey

AU - Gorceix, Nicolas

AU - Choi, Seonghwan

AU - Kellerer, Aglaé

AU - Cao, Wenda

AU - Goode, Philip R.

AU - Abramenko, Volodymyr

AU - Richards, Kit

AU - Rimmele, Thomas R.

AU - Marino, Jose

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N2 - 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.

AB - 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.

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ER -

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

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