15
DVA-1 Project Overview Gordon Lacy April 2014

DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

Embed Size (px)

Citation preview

Page 1: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

DVA-1 Project Overview

Gordon Lacy

April 2014

Page 2: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

The Dish Verification Antenna, DVA-1

• Key Features:• A 15m aperture, feed-high offset Gregorian with shaped optics• Rim supported composite shell primary and secondary• Composite tubes supporting feed platform and secondary• Deep tubular truss backing structure

Page 3: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

3

DVA-1: Designed for High Dynamic Range Capability

• High Thermal Performance• Rim supported monocoque design along with very low CTE materials keeps all

thermal movement both small and very uniform to minimize effect on beam pattern

• High Performance in Wind and Gravity• Central compliant connector allows some structural sag without inducing unwanted

distortion at center of dish

• Rim supported design keeps dish deflections to absolute minimum and concentrates any deflections at rim where effect on performance is small.

• Extremely deep truss back structure keeps dish shape as close to rigid as is possible.

• High Overall Optics Stability• Secondary and feed platform support optimized to maximize stiffness using shape

optimization software.

• Secondary and feed support tubes use zero and matched CTE carbon tubes for extremely high thermal stability.

Page 4: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

• Clear optical path, no blockage or scattering

• Combined with shaped optics, leads to very low spillover (~ -50db wide angle)• Very low spillover yields very low antenna noise temperature (<6 K ground)• Very low spillover results in high rejection of RFI and strong sources• Shaped optics yield high efficiencies, total result is a high Aeff / Tsys

DVA-1: Shaped Offset Optics Advantage

Page 5: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

DVA-1

Page 6: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

6

DVA-1: Composites for Performance

Structural Test Composite Design Consideration

Metallic Design Consideration

Creep high static load high static load

Static Strength Material properties Material properties

Fatigue Life High cyclic load High cyclic load

Glass Transition Temp. Choose resin with sufficiently high value.

NA

Impact Resistance Engineering requirement Engineering requirement

Galvanic Corrosion Encapsulate reflective layer Paint and primer

UV, Moisture, Humidity Paint (no primer required) and resin properties

Paint and Primer

Reflectivity Degradation Paint (no primer required) Paint and Primer

Fungus growth Paint Paint

Page 7: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

Recovery from Disaster

Page 8: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

Crack Repair

Page 9: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

DVA-1 Reflector Repairs

Page 10: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

DVA-1 Reflector Accuracy After Repairs

• Primary reflector RMS after repairs and without antenna weighting, 1.0mm

• RMS with repair areas removed, 0.7mm without antenna weighting

Page 11: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

DVA-1 Secondary Reflector Accuracy

•Secondary Part RMS without antenna weighting 0.2mm

•With antenna weighting 0.11mm

Page 12: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

GDSatcom Secondary Reflector

•We have now built two sub reflectors for the GDSatcom Meerkat project

•RMS of reflector 0.090mm

•Mold RMS 0.058mm

Page 13: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

13

DVA-1 Prototype Target:

To meet all of the SKA performance goals, as of Q4 2012.

2014 Target

To meet the SKA 2012 performance goals

To investigate the SKA 2014 low frequency requirements

To investigate the SKA 2014 high frequency requirements

Page 14: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

Questions?

Page 15: DVA-1 Project Overview Gordon Lacy April 2014. The Dish Verification Antenna, DVA-1 Key Features: A 15m aperture, feed-high offset Gregorian with shaped

1515

EndGordon Lacy, P.Eng. Tel: [email protected]