the details…
DESCRIPTION
The Details…. Previous Focus Tracking Curves. Previous Focus Tracking Curves. Temperature Sensor Locations. T F1. T F5. T SR. T F3. T F4. T F2. T H3. T B2. T H2. T E2. T B1. T B3. T B4. T B5. T E1. T A4. T A2. T A3. T A1. Structural Temperatures. Focus Model. Gravity - PowerPoint PPT PresentationTRANSCRIPT
1SPIE – June 25, 2004
The Details….
2SPIE – June 25, 2004
Previous Focus Tracking Curves
3SPIE – June 25, 2004
Previous Focus Tracking Curves
4SPIE – June 25, 2004
Temperature Sensor Locations
TSR
TF1
TF4
TF5
TF3
TF2
TH2
TH3 TB2
TB1 TB3
TB5
TB4
TE1
TE2
TA3
TA1
TA2
TA4
5SPIE – June 25, 2004
Structural Temperatures
6SPIE – June 25, 2004
Focus Model
• Gravity
• SR-Primary
• VFA-Primary
• HFA
• BUS
7SPIE – June 25, 2004
Elevation Model
• Gravity
• BUS
• HFA
• VFA
• Alidade
8SPIE – June 25, 2004
Azimuth Model
• Gravity
• Alidade
• HFA
• BUS
• VFA
9SPIE – June 25, 2004
Optimization
• Focus optimization using pseudo-inverse for LSE solution
• Coupled Az and El gravity models (AN, AW constraint)– Gradient descent
10SPIE – June 25, 2004
• 100 x 110 m section of a parent parabola 208 m in diameter• Cantilevered feed arm is at focus of the parent parabola
Unblocked Aperture
11SPIE – June 25, 2004
Telescope Structure and Optics
12SPIE – June 25, 2004
Development Phases
Actual schedule:
Phase I: ??
Phase IIa (26GHz) Spring 2003
13SPIE – June 25, 2004
High Frequency Environmental Envelope
14SPIE – June 25, 2004
Pointing Accuracy, 5° C Gradient, 5° El
Loral Tech Memo 52 Table 2-20 El=5, T=5,Vw=0,Sun Az=180
Error Sources El Errors (arcsec) X-El Errors (arcsec)Repeatable Nonrepeatable Repeatable Nonrepeatable
Mechanical AlignmentsRF/El Axes Orthogonality 0.0 0.0El/Az Axes Orthogonality 0.0 5.2Az Axis Verticality 5.0 0.4Structural DeformationsReflectorWindThermal Gradient 0.3AlidadeWind Thermal Gradient 11.5Servo and Drive 0.9 0.3MiscellaneousEl Bearing Wobble 1.0 0.4 0.1 0.0Az Bearing Wobble 1.0 0.4 0.1 0.0Encoder Accuracy 1.2 1.2Encoder Coupling 1.8 2.1Encoder Referencing 10.0 10.0RSS Subtotals 11.3 12.1 11.3 2.4
15SPIE – June 25, 2004
Pointing
16SPIE – June 25, 2004
Focus
17SPIE – June 25, 2004
Data Quality
Jack Scan
Gaussian Fits (Az, El, Focus)
Polarization (LCP – RCP)
Direction (Forward – Backward)
18SPIE – June 25, 2004
Data Quality: Pointing (LCP – RCP)
19SPIE – June 25, 2004
Structural Temperature Sensors
• 19 locations, 0.2C interchangeable accuracy, 0.01C resolution, 1Hz, range –35 to 40C. (actual accuracy is ~0.1C, temp control of conversion elex)
• Design documentation:– PTCS Wiki (AntennaInstrumentation) – PTCS Project Note PTCS/PN12
• Accuracy tested in lab:– Solar/convective loading– Selected unit-to-unit accuracy, repeatability– Electronics temperature range
• RFI mitigated, ESD protected• Two thermistor failures, forensics with YSI• Integrated into M&C • First cut pointing, focus predictive algorithms tested
20SPIE – June 25, 2004
Focus Model Tests
• Wind < 2.5 m/s• 15° < elevation < 85° • 9/5 is NCP • 11/20 is all-sky• Excludes 1000-1800• Graphs show thermal
contributions only
21SPIE – June 25, 2004
Elevation Model Test
22SPIE – June 25, 2004
Elevation Model Test
23SPIE – June 25, 2004
Azimuth Model
Term Coefficient Min-Max Significance Parameter
M1 5.5862 4.0 22.4 Alidade M2 -8.0331 2.7 21.3 HFAM3 -1.6289 2.4 3.8 BUSM4 1.3683 2.0 2.8 VFAM5 3.4124 0.0 0.0 CA, d(0,0)M6 1.3223 0.7 1.0 NPAE, b(0,1)M7 3.5152 0.9 3.0 IA, d(0,1)M8 -2.4960 1.9 4.8 AW, b(1,1)M9 -1.3360 1.8 2.5 AN, a(1,1)
24SPIE – June 25, 2004
Azimuth Model Estimation
= 3.9
25SPIE – June 25, 2004
Azimuth Model Test
26SPIE – June 25, 2004
Azimuth Model Test
27SPIE – June 25, 2004
Holography Results
Finite Element Model Predictions
29SPIE – June 25, 2004
Efficiency and Beam Shape
30SPIE – June 25, 2004
Requirements for high-frequency observing
31SPIE – June 25, 2004
Requirements for high-frequency observing
32SPIE – June 25, 2004
Pointing Accuracy, 6 m/s wind
Error Sources El Errors (arcsec) X-El Errors (arcsec)Repeatable Nonrepeatable Repeatable Nonrepeatable
Mechanical AlignmentsRF/El Axes Orthogonality 0.0 0.0El/Az Axes Orthogonality 0.0 35.3Az Axis Verticality 5.0 2.9Structural DeformationsReflectorWind 10.5Thermal Gradient AlidadeWind 1.5Thermal Gradient Servo and Drive 0.9 0.3MiscellaneousEl Bearing Wobble 1.0 0.4 0.6 0.2Az Bearing Wobble 1.0 0.4 0.6 0.2Encoder Accuracy 1.2 1.2Encoder Coupling 1.8 1.7Encoder Referencing 10.0 8.1RSS Subtotals 11.3 12.3 36.4 2.1
33SPIE – June 25, 2004
Architecture of current GBT Observing System
34SPIE – June 25, 2004
Architecture of HFOS
35SPIE – June 25, 2004
Architecture of PCS
36SPIE – June 25, 2004
Telescope Structure and Optics
•Optics: 110 m x 100 m of a 208 m parent paraboloid•Effective diameter: 100 m•Offaxis feedarm
•Elevation Limit: 5degrees•Slew Rates: Azimuth – 40deg/min; Elevation – 20deg/min•Main Reflector: 2209 actuated panels with 68 m rms.
•Total surface: rms 400 m•FWHM Beamwidth: 740"/f(Ghz)•Prime Focus: Retractable boom•Gregorian Focus:
•8-m subreflector with 6-degrees of freedom•Rotating Turret with 8 receiver bays