wind lidar working group, 29 june 2005 welches, or doppler lidar scanning telescope technology geary...

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Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space- based Lidar Winds Welches, Oregon June 28- July 1, 2005

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Page 1: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Doppler Lidar Scanning Telescope Technology

Geary Schwemmer

Meeting of the Working Group on Space-based Lidar Winds

Welches, Oregon

June 28- July 1, 2005

Page 2: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Topics

• Requirements

• Constraints

• Approaches

• Comparisons

• Roadmaps

Page 3: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Requirements

• Narrow field of view

• Large collecting area

• Large off-nadir scan angles (~30-50°)

• Step-stare preferred over continuous scanning

• Rapid slew

• 2 ~orthogonal looks into each sample volume

• Laser bore-sighting

Page 4: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Constraints

• Volume• Mass• Power• Vibration• Torque• Momentum compensation• Space environment

Page 5: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Approaches

• Conventional telescope w/ rotating mount

• Multiple telescopes

• Scanning flat mirror

• Rotating wedge prism

• Rotating Fresnel prism

• Rotating HOE

• Multiplexed HOE / SHADOE

Page 6: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Comparisons

Mass and Power comparisons. (Source - GSFC Doppler Lidar Technology assessment, 2001.)

System Total Mass Total Avg. Power

Rotating SiC 1.25 m reflective telescope

302 kg 260 W

Scanning flat mirror >450 kg

Rotating Fresnel wedge

>450 kg

Rotating 1.5-m HOE 152 kg 130 W

1.5-m ShADOE 65 kg 20 W

Page 7: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Holographic Optics

IR

Page 8: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Hybrid SHADOE Roadmap

TRL5TRL4

TRL3

Page 9: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Key Remaining Issues

• Space qualification• 2-micron performance

(diffraction limited)• SHADOE demonstration• System trades:

– laser– # of FOVs & dwell time / spatial

resolution– hybrid configuration

• Scaling to 1 meter

Page 10: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Conclusions

• Conventional scanning telescope too heavy• 2-micron & 355 nm requirements very

different (size & image quality), perhaps equally difficult

• HOE technologies offer significant weight and power savings for large apertures

• Perhaps the lowest TRL of UV Doppler components

• No show stoppers, but significant risk & development

Page 11: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

150°

Baseline Scan Configuration

Satellite nadir ground track

YA= 324 km

YB= 87 km

30°

Z = 400 km, = 40°, A = 75°, B = 15°, C = 45°

YC= 237 km 90°324 km

237 km

3 tracks, 6 lines of sight

0 90

seconds timing

12 7833 57

Page 12: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Optical Layout(single HOE)

Page 13: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

UV-A exposure effects

Page 14: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Wavefront Error Correction

Wave-front corrective

prescription applied to cover glass

Wave-front distortion caused by HOE materials

Page 15: Wind Lidar Working Group, 29 June 2005 Welches, OR Doppler Lidar Scanning Telescope Technology Geary Schwemmer Meeting of the Working Group on Space-based

Wind Lidar Working Group, 29 June 2005 Welches, OR

Hybrid R-T Combination SHADOE Receiver(One FOV shown)

UV Reflection SHADOE

IR Transmission SHADOE

IR Focal Plane

UV Focal Plane