HARLIE Winds: Methods and Results

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HARLIE Winds: Methods and Results M. Anderson, I. Andrus, C. Egbert, and T. Wilkerson Space Dynamics Laboratory Utah State University, Logan, UT 84341 (435) 797-9611 [email protected] Presentation for Working Group on Space-Based Lidar Winds Key West, FL January 23-25,2002

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HARLIE Winds: Methods and Results. M. Anderson, I. Andrus, C. Egbert, and T. Wilkerson Space Dynamics Laboratory Utah State University, Logan, UT 84341 (435) [email protected] Presentation for Working Group on Space-Based Lidar Winds Key West, FLJanuary 23-25,2002 - PowerPoint PPT Presentation

Transcript of HARLIE Winds: Methods and Results

Page 1: HARLIE Winds: Methods and Results

HARLIE Winds: Methods and Results

M. Anderson, I. Andrus, C. Egbert, and T. Wilkerson

Space Dynamics Laboratory

Utah State University, Logan, UT 84341(435) 797-9611 [email protected]

Presentation for Working Group on Space-Based Lidar Winds

Key West, FL January 23-25,2002

* Research Support: NPOESS, NASA, and SDL

Page 2: HARLIE Winds: Methods and Results

Research Objectives

• Develop methods for HARLIE wind profiling

• Compare HARLIE results with other wind sensors (sondes, GLOW, cloud imagery)

• Refine techniques for data visualization and analysis

• Develop mature HARLIE capability for wind lidar Cal/Val

Page 3: HARLIE Winds: Methods and Results

HARLIE Winds: Methods and Results

Wave image of HARLIE conical scan data: Curve-fit method

Video imagery of cloud motions: Automated pattern recognition and tracking

Automated data reduction for HARLIE scans

• Plans and directions for future work

Topics

Page 4: HARLIE Winds: Methods and Results

Available Wind Data Comparisons (HARGLO-2)

HARLIE(Automated)

HARLIE(Manual)

SkyCam(Automated)

Sondes GLOW

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HARLIE Wave Image Wind direction and speed

Lidar return as a function of HARLIE scan angle and time

Curve fit(Manual/Automated)Phase directionAmplitude speed

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HARGLO-2 Nov. 16, 2001

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LORAN Sonde 11:00 UT to 12:37 UT HARLIE Manual 11:00 UT to 11:30 UT

HARLIE Manual 12:00 UT to 12:30 UT

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HARGLO-2 Nov. 17, 2001

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Cloud tracking via Block Matching (camera image space)

Cloud feature identification Wind Speed and Direction(includes camera distortion correction)

Page 9: HARLIE Winds: Methods and Results

Previous cloud tracking method (manual)

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Test of cloud-tracking algorithm from ARM-CART site campaign Oct. 4, 2000

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Wind Gradients March 7, 1999

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SkyCam

Page 12: HARLIE Winds: Methods and Results

Graphical Representation of the Automatic Curve Fit Routine

Intensity vs. Rotation 3/ 9/ 99 13:00 UT

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Wind Velocity and Direction17 Nov, 2001

17 Nov 2001 1700-1729 UT

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HARLIE Automatic HARLIE Manual Sky Cam

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Wind Velocity and Direction 19 Nov, 2001

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HARGLO-2 Nov. 19, 2001

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LORAN Sonde 11:00 to 12:22 Harlie Manual 11:00 to 11:30 Harlie Manual 11:22 to 12:08

Harlie Manual 11:52 to 12:38 Harlie Automatic 11:30 to 12:00 Harlie Automatic 12:00 to 12:30

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Direction (deg)

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GLOW and HARLIE (preliminary results)HARGLO-2

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HARLIE - manual data extraction GLOW SkyCam

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Status and Plans (USU)

• Automated HARLIE data reduction works• Automated cloud tracking works• These methods still undergoing critical tests• Complete reduction/comparison of

HARGLO-2 data• Additional methods being explored

(correlation/ Fourier analysis)• New measurement campaigns under

consideration

Page 18: HARLIE Winds: Methods and Results

HARLIE Winds: Methods and Results

M. Anderson, I. Andrus, C. Egbert, and T. Wilkerson

Space Dynamics Laboratory

Utah State University, Logan, UT 84341(435) 797-9611 [email protected]

Presentation for Working Group on Space-Based Lidar Winds

Key West, FL January 23-25,2002

* Research Support: NPOESS, NASA, and SDL