2017
DOI: 10.1088/1538-3873/129/973/035001
|View full text |Cite
|
Sign up to set email alerts
|

Thermal, Structural, and Optical Analysis of a Balloon-Based Imaging System

Abstract: Abstract. The Subarcsecond Telescope And BaLloon Experiment, STABLE, is the fine stage of a guidance system for a high-altitude ballooning platform designed to demonstrate subarcsecond pointing stability, over one minute using relatively dim guide stars in the visible spectrum. The STABLE system uses an attitude rate sensor and the motion of the guide star on a detector to control a Fast Steering Mirror in order to stabilize the image. The characteristics of the thermal-optical-mechanical elements in the syste… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
3
0

Year Published

2017
2017
2024
2024

Publication Types

Select...
6
2

Relationship

0
8

Authors

Journals

citations
Cited by 15 publications
(6 citation statements)
references
References 14 publications
0
3
0
Order By: Relevance
“…For some large-scale optical instruments, increased fine finite element meshing is usually required [76]. Banyal et al proved that a higher order Zernike polynomial also has a certain influence on the fitting of optical surfaces [37].…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…For some large-scale optical instruments, increased fine finite element meshing is usually required [76]. Banyal et al proved that a higher order Zernike polynomial also has a certain influence on the fitting of optical surfaces [37].…”
Section: Discussionmentioning
confidence: 99%
“…The rigid body displacement of the primary mirror was separately input into the optical analysis in IOA; thus, the optical surface deformation that removes the rigid body displacement was fitted. Zernike polynomials select the 34-term polynomials that remove the tip/tilt/piston terms [76]. Based on the 34-term Zernike polynomial, the input of 1D-CNN is 34 terms, and the output is a node sag change.…”
Section: The Potential For Ann Use In Ioamentioning
confidence: 99%
“…Fitting Interpolation To date, this method has been applied to the design of optical instruments such as space optical instruments and large ground-based telescopes, and it is used to evaluate whether the optical performance of optical systems fulfills the requirements under the action of mechanical/thermal environmental loads [15][16][17][18][19][20]. The characteristics of the thermaloptical-mechanical elements in the Subarcsecond Telescope and BaLloon Experiment (STABLE) directly affect the quality of the point-spread function of the guide star on the detector, so a series of thermal, structural, and optical models were built to simulate system performance and ultimately inform the final pointing stability predictions [15].…”
Section: Interface Programs Zernikementioning
confidence: 99%
“…Fitting Interpolation To date, this method has been applied to the design of optical instruments such as space optical instruments and large ground-based telescopes, and it is used to evaluate whether the optical performance of optical systems fulfills the requirements under the action of mechanical/thermal environmental loads [15][16][17][18][19][20]. The characteristics of the thermaloptical-mechanical elements in the Subarcsecond Telescope and BaLloon Experiment (STABLE) directly affect the quality of the point-spread function of the guide star on the detector, so a series of thermal, structural, and optical models were built to simulate system performance and ultimately inform the final pointing stability predictions [15]. During the development process of projects such as the Laser Interferometer Space Antenna (LISA) [16], Wide-Field Infrared Survey Telescope (WFIRST) [17], Narrow-Field Infrared Adaptive Optics System (NFIRAOS) [18], 4 m telescope for habitable exoplanet observation mission (HabEx) [19], and Advanced Terrain Laser Altimeter System (ATLAS) [20] in the ICESat-2 mission, an optical mechanical thermal integration analysis model was established, and the analysis results were validated for the system design.…”
Section: Interface Programs Zernikementioning
confidence: 99%
“…The Pareto diagram shows that the only architecture capable to fulfill the thermal and stiffness requirements is the number 11.1 corresponding to a hexapod composed by 6 shafts. This architecture is an extrapolation of a trivial hexapod used to sustain large structures like mirrors of telescope or other optical devices ( [6], [7], [8]).…”
Section: Chania Greece 9 -12 October 2018mentioning
confidence: 99%