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Understanding the ULB-2000 Integrating Sphere

Table of Contents

Introduction to Integrating Sphere Technology

Integrating spheres are fundamental optical components used in radiometric, photometric, and spectroradiometric measurements. Their primary function is to provide uniform spatial distribution of light, ensuring accurate and repeatable measurements of luminous flux, colorimetric parameters, and spectral power distribution. The ULB-2000 Integrating Sphere, when paired with the LPCE-3 Spectroradiometer System from LISUN, forms a high-precision solution for industries requiring stringent lighting performance evaluations.

This article explores the technical principles, specifications, and applications of the ULB-2000 sphere in conjunction with the LPCE-3 system, emphasizing its role in industries such as LED/OLED manufacturing, automotive lighting, aerospace, and medical lighting.


Design and Operational Principles of the ULB-2000 Integrating Sphere

Optical Configuration and Coating Properties

The ULB-2000 employs a highly reflective barium sulfate (BaSO₄) coating, ensuring >95% diffuse reflectance across the visible spectrum (380–780 nm). This minimizes absorption losses and maximizes light homogenization, critical for precise spectroradiometric measurements. The sphere’s internal baffle system prevents direct illumination of the detector, reducing measurement artifacts.

Mathematical Basis of Integrating Sphere Theory

The radiant flux (Φ) measured within an integrating sphere follows the equation:

[
Phi = frac{E cdot A_{text{detector}}}{rho cdot (1 – rho(1 – f))}
]

Where:

  • (E) = Irradiance at the detector (W/m²)
  • (A_{text{detector}}) = Detector area (m²)
  • (rho) = Reflectance of the sphere coating
  • (f) = Port fraction (ratio of open area to total sphere surface)

The LPCE-3 system leverages this principle to derive luminous flux (lm), chromaticity coordinates (CIE 1931/1976), correlated color temperature (CCT), and color rendering index (CRI) with high repeatability.


Integration with the LPCE-3 Spectroradiometer System

Key Specifications of the LPCE-3 System

Parameter Specification
Spectral Range 380–780 nm (extendable to 200–1100 nm)
Wavelength Accuracy ±0.3 nm
Photometric Linearity ±0.3%
CRI Measurement Range 0–100 (Ra, R1–R15)
Luminous Flux Accuracy ±3% (Class A)
Detector Type High-sensitivity CCD array

The LPCE-3 system complies with CIE 177, CIE 13.3, IES LM-79, and EN 13032-1 standards, making it suitable for regulatory testing in multiple industries.

Testing Workflow

  1. Calibration – A NIST-traceable standard lamp calibrates the system, ensuring traceability.
  2. Sample Mounting – The light source is positioned at the sphere’s input port, avoiding obstructions.
  3. Data Acquisition – The LPCE-3 spectroradiometer captures spectral data, processed via LISUN’s LMS-9000 software for real-time analysis.
  4. Reporting – Automated reports generate metrics such as PPFD (Photosynthetic Photon Flux Density) for horticultural lighting or MEL (Melanopic Lux) for human-centric lighting.

Industry-Specific Applications

1. LED and OLED Manufacturing

The ULB-2000/LPCE-3 system verifies binning consistency, angular color uniformity, and long-term flux depreciation in LED production lines. For OLEDs, it measures emission spectra and efficiency under varying drive currents.

2. Automotive Lighting Testing

Compliance with UNECE R37, SAE J578, and FMVSS 108 requires precise luminous intensity and chromaticity validation. The LPCE-3 system evaluates headlamps, taillights, and interior ambient lighting for glare, color shift, and thermal stability.

3. Aerospace and Aviation Lighting

Aircraft lighting must meet RTCA DO-160 standards for electromagnetic interference and luminance uniformity. The integrating sphere tests cockpit displays, emergency lighting, and navigation lights under simulated altitude conditions.

4. Medical Lighting Equipment

Surgical and diagnostic lighting requires flicker-free operation and high CRI (Ra > 90). The LPCE-3 quantifies blue light hazard (IEC 62471) and flicker percentage (IEEE 1789).

5. Photovoltaic Industry

The system measures solar simulator spectral mismatch per IEC 60904-9, ensuring accurate PV cell efficiency testing.


Competitive Advantages of the LPCE-3 System

  1. Multi-Standard Compliance – Supports IES, CIE, ANSI, and ISO requirements in a single platform.
  2. Modular Expandability – Optional accessories include goniophotometers and environmental chambers for stress testing.
  3. Automated Workflows – Reduces operator dependency via pre-programmed test sequences.
  4. High Dynamic Range – Capable of measuring 0.1–200,000 lux without external attenuation.

FAQ Section

Q1: What is the recommended calibration interval for the LPCE-3 system?
A: Annual calibration is advised, with quarterly verification checks using a reference source.

Q2: Can the ULB-2000 measure pulsed or flickering light sources?
A: Yes, the LPCE-3 supports high-speed sampling (up to 20 kHz) for PWM and transient light analysis.

Q3: How does the LPCE-3 handle UV and IR measurements?
A: With an extended-range spectrometer (200–1100 nm), it quantifies UV irradiance (ISO 21348) and near-IR efficacy for specialized applications.

Q4: Is the system suitable for flexible OLED testing?
A: Yes, a specialized holder prevents mechanical stress during bendable OLED evaluations.

Q5: What file formats are supported for data export?
A: CSV, PDF, and XML formats are available for integration with SPC and LIMS systems.


This technical overview underscores the ULB-2000 and LPCE-3 system’s role in advancing precision lighting measurement across diverse sectors. By adhering to international standards and leveraging high-fidelity optical design, the solution ensures reliability in both R&D and quality control environments.

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