Big Bear Solar Observatory NST Main Features All reflecting, off-axis Gregory optical configuration PM: 1.6 m clear aperture with f/2.4 Figuring PM to 16 nm rms Effective focal length: 83.2 m (F/52 at Gregorian focus) FOV: 3' in prime focus Wavelength range from 380 nm to 1.7 µm in Coudé lab with AO PM active thermally controlled Integrated active optics (ao) and adaptive optics (AO) Quasi-static telescope alignment Diffraction limited: 0.06″@ 500 nm and 0.2″@ 1.56 m with AO
10
Embed
Big Bear Solar Observatory NST Main Features All reflecting, off-axis Gregory optical configuration PM: 1.6 m clear aperture with f/2.4 Figuring.
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Big Bear Solar Observatory
NST Main Features All reflecting, off-axis Gregory
optical configuration PM: 1.6 m clear aperture with f/2.4 Figuring PM to 16 nm rms Effective focal length: 83.2 m (F/52
at Gregorian focus) FOV: 3' in prime focus Wavelength range from 380 nm to
1.7 µm in Coudé lab with AO PM active thermally controlled Integrated active optics (ao) and
I. Nasmyth Focus Filtergraph First-light scientific instrument Serves as scientific analysis and
engineering feedback Nasmyth prime focus Local correlation tracker (tip/tilt) FOV: 70″by 70″(square) Visible photometry
PCO camera 2K by 2K TiO 705.7 nm BF, FWHM 10 Å G-band 430.5 nm BF, FWHM 5.0 Å H Lyot NF, FWHM 0.25 Å Ca II K 393.3 nm NF
Near infrared photometry Rockwell camera 1K by 1K 1.6 m BF, FWHM 25 Å (deep layer) 2.23 m BF (cold clouds) 1.083 m NF (corona hole)
I
Big Bear Solar Observatory
First-light Scientific
Observations
Courtesy : F. Wőger and KISIP v.6
TiO 705.7 nm, FWHM 10 Å quiet sun H, FWHM 0.25 Å blue wing
Big Bear Solar Observatory
III. Adaptive Optics (AO) AO-76 which was used for BBSO
65 cm telescope, is a collaboration with NSO (T. Rimmele)
Shack Hartmann WFS with 76 sub-apertures (AO-76)
Xinetics Deformable Mirror with 97 actuators
High speed Baja camera with a frame rate of 2500 frame/s
Bitware Hammerhead Boards with 40 digital signal processors (DSPs)
Closed-loop Bandwidth: 120 Hz Strehl ratio: 0.7 in the NIR under
median BBSO seeing
Big Bear Solar Observatory
III. Adaptive Optics (AO76)
Big Bear Solar Observatory
III. Adaptive Optics System
What’s Next ? AO-76 transition from BBSO 65 cm to NST AO-76 installation, calibration and optimization AO-76 routine operation for NIR and visible observation
Strehl ratio: 0.7 in the NIR under median BBSO seeing
AO-308 system development in collaboration with NSO Wave front sensor design, upgrade control system, matrix
reconstruction Streho ratio: 0.8 in the NIR under median BBSO seeing Strehl ratio: 0.35 in the visible under median BBSO seeing
AO-308 installation, calibration and optimization AO-308 routine operation for NIR and visible observation MCAO development in collaboration with NSO and
KIS Courtesy : T. Rimmele
AO-76
AO-308
VIS NIR
VIS NIR
Big Bear Solar Observatory
IV. IR Imaging Magnetograph NIR Fabry-Pérot etalon plus Lyot
filter and interference filter Wavelength coverage: 1 – 1.7 m Band pass: 10 pm Telecentric optical configuration Field of view: 75” by 75” Available spectral lines:
Fe I 15648.5 Ǻ Fe I 15652.9 Ǻ
Polarimeter: rotating wave plate ahead of M3
Spectrometric cadence: < 15 s Polarimetric cadence: < 2 min
Big Bear Solar Observatory
V. Visible Imaging Spectrometer Single Fabry-Pérot etalon plus
narrow band interference filter Spectrometer before NST AO-308
installation Wavelength coverage: 550 – 700 nm Band pass: 7.2 pm Telecentric optical configuration Field of view: 45” by 45” Available spectral lines:
H(656.3 ± 0.15 nm ) Fe I (630.2 ± 0.15 nm) NaD2 (588.9 ± 0.15 nm )
Cadence: < 15 s
Courtesy : C. Denker and A. Verdoni
Big Bear Solar Observatory
VI. FISS FISS – Fast Imaging Solar
Spectrograph A collaboration between BBSO and
Korean Solar Community Focus on fine structures of