Through A Glass Darkly Goals T ec hnical Approac h · Darkly The Laser Line-Scanner Pro ject Dr....

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* Near-field multiply scattered light Detector FOV Laser Off-axis light, Scattering losses Sunlight * illumination detector scattered into 0.0001 0.001 0.01 0.1 1 10 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5 Model 10m MCML 10m Model 2m MCML 2m

Transcript of Through A Glass Darkly Goals T ec hnical Approac h · Darkly The Laser Line-Scanner Pro ject Dr....

Page 1: Through A Glass Darkly Goals T ec hnical Approac h · Darkly The Laser Line-Scanner Pro ject Dr. Jonathan Stott (NU), Prof. W. Clem Karl (BU), Prof. Eric Miller (NU), and Prof. Charles

Through A Glass Darkly

The Laser Line-Scanner Project

Dr. Jonathan Stott (NU), Prof. W. Clem Karl (BU),

Prof. Eric Miller (NU), and Prof. Charles DiMarzio (NU)

Goals

Our goal is to improve the performance of theRaytheon laser line scanner (LLS).

* Near-field multiply scattered light

Detector FOV Laser

Off-axis light,

Scattering losses

Sunlight

*

illumination

detector scattered into

Signi�cance

� Ocean- oor sea mine detection

� Environmental monitoring

� Data inversion and sensor fusion

Technical Approach

Phase One|Model Light Propagation

Physics based signal processing

1. Radiative transport equation (RTE)

(k̂ � ~r)L(~r; k̂) =

��L(~r; k̂) + �

Zd

k̂0

4�f(k̂; k̂0)L(~r; k̂0)

� Very accurate, but diÆcult to solve.

� From RTE, make intuitive assumptions anddevelop model for the propagation of laserlight under the surface of the ocean.

� Model includes the e�ects of sunlight andnear-�eld multiply scattered light.

2. Monte Carlo calculations

� Few simplifying assumptions necessary.

� Potentially accurate, but very slow (preci-sion proportional to number of photons).

3. Validate RTE-based model against Monte Carlo.

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Model 10m MCML 10m

Model 2m MCML 2m

Comparison between our �rst-order model

predictions and Monte Carlo calculations of

the beam spread function.

Page 2: Through A Glass Darkly Goals T ec hnical Approac h · Darkly The Laser Line-Scanner Pro ject Dr. Jonathan Stott (NU), Prof. W. Clem Karl (BU), Prof. Eric Miller (NU), and Prof. Charles

Phase Two|Imaging

� Want to measure �(~r ), the re ectivity of theocean oor.

� Signal seen at the detector y(~r ) is

y(~r ) =

Z ZK(~r;~r 0)�(~r 0) d2~r 0 + �(~r )

where K(~r;~r 0) is the imaging kernel and �(~r ) isthe noise term.

� Assume translational invariance

� Reconstruct target re ectivity

{ Back-projection

{ Deconvolution

{ Wiener �lter

Synthetic Data

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1|Data−Reconstruction|

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Demonstration of image reconstruction

using noisy synthetic data.

Relation to CenSSIS

� SeaBED: �rst CenSSIS project with proprietaryfunding (Raytheon).

� Fundamental physics used to generate forwardmodel for light propagation.

� Physical model, in turn, improves image recon-struction algorithms of LLS.

� Work between the di�erent sites (NU and BU)coordinated via email/www and through regularface-to-face meetings.

Other Connections

� Work on di�usive wave imaging feeds in tomodeling of near-�eld multiply scattered light.

� Techniques from hyperspectral imaging (e.g.principal component analysis) are relevant for fu-ture work on improving LLS imaging by integra-tion of existing uorescence channels.

Current Status

� Forward model has been developed and is nowbeing validated against experimental data.

� Work on image reconstruction is on-going.

� Project is currently funded through June, 2000.Proposal for continuing funding submitted.

PI Contact Information

Name Charles DiMarzioTitle Principal Research Scientist

Institution Northeastern UniversityAddress FR 235

360 Huntington Ave.Boston, MA 02115

Phone (617) 373-2034Fax (617) 373-8627Email [email protected]

Plans and Project Evolution

Future

2Q 2000and beyond

1Q 2000

3Q and 4Q 1999Forward Model

ImageFormation

AdvancedHardware

LaserSources Configurations

Detector

ImageReconstruction

ClassificationLocalization

DetectionChannelFusion

(Fluorescence)