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GW-NH Status 25 January 2002.

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Presentation on theme: "GW-NH Status 25 January 2002."— Presentation transcript:

1 GW-NH Status 25 January 2002

2 GW-NH Status Overview Facility Update Facility Plans Science Update
Science Plans Operation Plans

3 GW-NH Status Facility Update

4 Facility Update MWO Bartlett Research Facility

5 Facility Update Structural fine-tuning of the instrument has been performed for ease of operation Telescope bearings tightened Laser table legged and bolted Support column vertically stabilized Dome replaced

6 Facility Update Laser Table Legged and Bolted

7 Facility Update Support Column Vertically Stabilized

8 Facility Update Telescope Bearings Tightened

9 Facility Update Dome Removal

10 Facility Update Dome Placement

11 Facility Update Dome Components

12 Facility Update Dome Shutter Motor

13 Facility Update Control Systems
Various control systems have been modified Dome control system rewired and reprogrammed Etalon controller noise/jitter suppressed

14 Facility Update Laser Laser seeding issues Laser issues
Thermal monitoring Replaced cable Replaced Piezo motor Laser issues Replaced trigger board Replaced power supply Reworked Pockels cell cable

15 GW-NH Status Facility Plans

16 Facility Plans Re-Integration
Resolve laser seeding issue ASAP Full re-integration (1-week) Replace motion controller Implement fiber optic alignment system (FOAS) Test etalon controller noise reduction Post re-integration campaign (1-week) Full utilization of system to test performance Comparison with radiosondes

17 GW-NH Status Science Update

18 Science Update Turbulence Investigation (J. McHugh)
Turbulence extraction algorithm is maturing Results look promising Awaiting new data to quantify the effects of noise reduction

19

20 GroundWinds AFRL

21 Science Update Spectral Investigations (Q. Zheng & J. Ryan)
Spectral broadening model Rayleigh scattering Brillouin scattering Turbulence (Instrument function) Information in broadened spectra Temperature Pressure Kinetic energy dissipation Aerosol-molecular ratio

22 Science Update PBL Investigations (J. Slater & M. Prentice)
PBL can be characterized by A/M profile PBL height and movement information Extinction and visibility information A and M decomposition requires a rigorous Aerosol scattering model Molecular scattering model Turbulence broadening model Instrument model

23 Science Update PBL Investigations (J. Slater & M. Prentice)

24 GW-NH Status Science Plans

25 Science Plans Mount Washington Valley Survey (J. McHugh)
Perform sweeps over the valley at different times of day and year to characterize Turbulent regions Gravity waves Flow features over MT. Washington Diurnal and seasonal patterns Fundamental modes

26 Science Plans Laser-Flow Interaction Studies (J. McHugh)
Fluid effects on laser Wavefront deformation Attenuation Beam steering Beam divergence Laser effects on fluid Local heating Generation of acoustic waves

27 Science Plans Depolarization Ratio Measurements
Measure the depolarization ratio of the backscattered beam Depolarization ratio profile will help quantify the composition, size, and shape of aerosols Distinguish ice, water, and dust

28 Science Plans Depolarization Ratio Measurements

29 Science Plans Depolarization Ratio Measurements

30 Science Plans Instrument Optimization
Determine the optimum GW setup for a given investigation Timing Altitude binning Azimuth angle/sweep rate Time of day/year Feasibility studies

31 GW-NH Status Operation Plans

32 Operation Plans Goal: 50% up-time Implement science plans
Web-based form for outside investigators General science objective Specific science objective GW-NH data product GW-NH setup (timing, altitude binning, etc.) Collaborating personnel


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