Optimization Analysis

Depth Detector Analysis

Depth distribution, local absorption, and field enhancement analysis

This page covers Normalized Poynting Vector, Absorption Density, Electric Field, and Refractive Index. This detector group is used for in-layer position analysis. System-level results belong to Basic Optical Results. Layer-level absorption attribution belongs to RTA and Layer Absorption Analysis.

Relevant result pages:

Prerequisites

ConditionCurrent requirement
Detector activationEnable the required detector in Optics > Depth Distribution
CoherenceNormalized Poynting Vector, Absorption Density, and Electric Field require a fully coherent stack
Depth ResolutionSet after enabling depth detectors; controls the number of depth samples
Analysis entryRun and Run Sweep
Direct optimizationDepth quantities are not direct optimization targets in the current implementation

Detector Roles

DetectorMain informationPrimary use
Normalized Poynting Vectornormalized energy flow along depthenergy transport and interface-to-interface flow change
Absorption Densitylocal dissipation strengthabsorption location and parasitic-loss location
Electric Fieldspatial distribution of field magnitude or phasestanding-wave nodes, field enhancement, interface-mode localization
Refractive Indexdepth-expanded refractive-index backgroundcomparison against layer boundaries and heatmap zones

Application Scope

ScenarioPrimary resultsRecommended sweeps
Parasitic-absorption localizationAbsorption Density, Layer Absorptionwavelength window, thickness
Cavity field enhancementElectric Fieldwavelength window, thickness, incidentAngle
Interface modes, defect modes, cavity modesElectric Field, Normalized Poynting Vectorwavelength window, incidentAngle, pRatio
Standing-wave node and antinode inspectionElectric Fieldwavelength window, thickness
Post-optimization validationdepth detectors + R / T / Aoptimize first, then inspect local behavior

Baseline Model

Structure

This example keeps the same ITO 40 nm + Substrate 1 um stack. As in the ellipsometry section, the full stack remains coherent to make in-layer field distributions available.

Single-Wavelength Optical Parameters

ItemSetting
Wavelength SamplingSingle
Wavelength550 nm
Incident Angle
pRatio0.5
Base detectorsReflectance, Layer Absorption
Depth detectorsNormalized Poynting Vector, Absorption Density, Electric Field, Refractive Index
Depth Resolution10 nm

Wavelength-Sweep Optical Parameters

ItemSetting
Wavelength SamplingSweep
Wavelength range400-900 nm
Step20 nm
Incident Angle
pRatio0.5
Depth Resolution10 nm

Single Run

Electric Field Line Chart

This figure corresponds to a single wavelength with no Sweep parameter. The horizontal axis is depth, and the shaded regions mark layer boundaries. It is used to read:

  • node and antinode positions
  • whether the target layer sits in a high-field region
  • whether local enhancement appears near an interface

In this example, the ITO layer is thin and the main oscillation sits in the substrate region. This is a good baseline for deciding whether thickness sweeps are necessary.

Normalized Poynting Vector Line Chart

This chart shows that normalized energy flow stays nearly flat along depth for each thickness, with different thickness values shifting the overall level. It is used to read:

  • whether energy transport remains smooth across the stack
  • whether some thickness values introduce extra flow loss

Normalized Poynting Vector is most useful together with Absorption Density. By itself it does not locate where absorption happens.

One-Parameter Sweep

Sweep Setup

ParameterFromToStep
structure/ITO/thickness2012020

Electric Field Heatmap

This chart is fixed at 560 nm. The horizontal axis is depth and the vertical axis is ITO thickness. It is used to read:

  • whether nodes and antinodes shift with thickness
  • whether the high-field region moves into the target layer
  • which thickness ranges produce a more stable spatial distribution

The heatmap is the primary depth view for one-parameter sweeps. It is better than a line chart for comparing multiple stacks.

Electric Field 3D Scatter

This chart keeps wavelength, depth, and ITO thickness as axes. It is used to read:

  • whether field enhancement persists along a wavelength-thickness trajectory
  • whether extrema are isolated hot spots or continuous ridges
  • whether resonance locations shift systematically with thickness

The 3D scatter is a trend-inspection tool. Exact positions should still be checked in line or heatmap views.

Absorption Density Heatmap

In this baseline stack the local absorption density is near zero, so the map is close to a uniform background. This figure is still useful because it establishes two rules:

  • Absorption Density only becomes visually strong when the stack contains significant local dissipation
  • a nearly uniform map should trigger a back-check in Absorptance and Layer Absorption, not an automatic assumption of error

A flat depth heatmap can simply mean that the baseline structure has weak local loss in the current band.

Relation to Layer Absorption

Results pageResolution levelPrimary role
Layer Absorptionby layeridentify which layer absorbs
Absorption Densityinside a layeridentify where inside that layer absorption occurs
Electric Fieldfield distributioncheck whether absorption overlaps with a high-field region

Recommended order:

  1. Use Absorptance to confirm that significant total absorption exists.
  2. Use Layer Absorption to identify the layer of interest.
  3. Use Absorption Density and Electric Field to locate the in-layer position and the field-enhancement region.
GoalRecommended order
Locate local absorptionLayer AbsorptionAbsorption Density heatmap → Electric Field
Inspect interface or cavity modesReflectance or spectral results → Electric Field heatmap → Electric Field 3D scatter
Post-optimization validationOptimization ReportR / T / A → depth results

Relation to the Optimizer

ItemCurrent status
direct optimization on depth quantitiesNot supported
recommended usephysical validation after optimization

Depth detectors belong after the optimizer in the current workflow. First use R / T / A to identify candidate structures. Then use depth results to validate whether the local physical picture is acceptable.

Conclusion Boundaries

  • Depth detectors apply to internal field analysis in one-dimensional layered stacks.
  • The current results must not be used to explain lateral patterns, scattering structures, or general 2D / 3D mode problems.
  • Refractive Index is primarily a structural background view, not a standalone performance metric.

Case Study Entry

For full structures and workflows, see Case Studies. Future cases will cover parasitic-absorption localization, interface modes, cavity-enhanced absorption, and post-optimization depth validation.

Next Step

The current Analysis chapter now covers the three main detector groups. Continue with Case Studies for full application workflows.

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