1 / 15

Doppler Lidar Scanning Telescope Technology

Doppler Lidar Scanning Telescope Technology. Geary Schwemmer Meeting of the Working Group on Space-based Lidar Winds Welches, Oregon June 28- July 1, 2005. Topics. Requirements Constraints Approaches Comparisons Roadmaps. Requirements. Narrow field of view Large collecting area

hattiek
Download Presentation

Doppler Lidar Scanning Telescope Technology

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


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

  2. Topics • Requirements • Constraints • Approaches • Comparisons • Roadmaps

  3. 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

  4. Constraints • Volume • Mass • Power • Vibration • Torque • Momentum compensation • Space environment

  5. Approaches • Conventional telescope w/ rotating mount • Multiple telescopes • Scanning flat mirror • Rotating wedge prism • Rotating Fresnel prism • Rotating HOE • Multiplexed HOE / SHADOE

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

  7. IR UV Holographic Optics

  8. Hybrid SHADOE Roadmap TRL3 TRL4 TRL5

  9. 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

  10. 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

  11. Baseline Scan Configuration 3 tracks, 6 lines of sight 237 km 30° YA= 324 km YB= 87 km 150° Satellite nadir ground track 324 km 90° YC= 237 km 0 12 78 90 33 57 seconds timing Z = 400 km,  = 40°, A = 75°, B = 15°, C = 45°

  12. Optical Layout(single HOE)

  13. UV-A exposure effects

  14. Wavefront Error Correction Wave-front distortion caused by HOE materials Wave-front corrective prescription applied to cover glass

  15. Hybrid R-T Combination SHADOE Receiver(One FOV shown) UV Focal Plane UV Reflection SHADOE IR Transmission SHADOE IR Focal Plane

More Related