ASTM E424 Test Methods for Solar Energy Transmittance and Reflectance (Terrestrial) of Sheet Materials

ASTM E424 test procedure includes two test techniques for measuring solar energy transmittance and reflectance (terrestrial) in sheet materials. The heat transmission through fenestration, most often glass or plastics, is regulated by solar-energy transmittance and reflectance.

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    ASTM E424 Test Methods for Solar Energy Transmittance and Reflectance (Terrestrial) of Sheet Materials

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    • Overview
    • Scope, Applications, and Benefits
    • Test Process
    • Specifications
    • Instrumentation
    • Results and Deliverables

    Overview

    ASTM E424 is a fundamental standard for assessing the solar-optical characteristics of sheet materials, including glass, plastic glazing, and films.  It provides a baseline for determining how much solar energy is transmitted or reflected by various materials under terrestrial conditions. It was established in 1971 and has been periodically reapproved (most recently in 2023).

    The purpose of the standard is to quantify the reflectance and transmittance of solar energy. When assessing the “heat admission” through fenestration (windows, skylights) and the effectiveness of solar collectors, engineers and architects rely heavily on these measurements.

    Scope, Applications, and Benefits

    Scope

    ASTM E424 specifies test methods for determining the solar energy transmittance and reflectance of sheet materials under terrestrial solar radiation conditions. The test evaluates the amount of incident solar energy transmitted through or reflected from materials when exposed to sunlight representative of natural outdoor conditions. It is applicable to transparent, translucent, and reflective sheet materials used in architectural, automotive, aerospace, and solar-related applications, supporting assessment of their thermal and energy performance.

    Applications

    • Architectural glazing, windows, skylights, and façade materials
    • Solar control films and reflective coatings
    • Automotive and transportation glazing materials
    • Aerospace and defense thermal management materials
    • Building energy modeling and compliance assessments
    • Research and development of solar and energy-efficient materials

    Benefits

    • Enables accurate evaluation of solar energy transmission and reflection characteristics
    • Supports energy-efficiency analysis of materials exposed to sunlight
    • Helps in material selection for thermal control and solar management
    • Provides standardized, repeatable results for quality control and R&D
    • Assists in predicting heat gain and optical performance under real-world conditions

    Testing Process

    Specimen Preparation

    Cut and clean sheet material specimens to specified dimensions; condition as required.

    1

    Instrument Setup

    Set up a spectrophotometer or solar measurement system as per ASTM E424 requirements.

    2

    Calibration

    Calibrate the instrument using standard reference materials

    3

    Reporting

    Report results with test conditions and specimen details.

    4

    Technical Specifications

    ParameterDetails
    Measurement MethodSpectrophotometric measurement of transmittance and reflectance
    Spectral RangeSolar spectrum (UV–Vis–NIR region)
    Test InstrumentUV–Vis–NIR spectrophotometer with integrating sphere
    CalibrationUse of certified reflectance/transmittance standards
    Test OutputSolar energy transmittance and reflectance values
    Sample TypeSheet materials (transparent or translucent)

    Instrumentation Used

    • UV–Vis–NIR spectrophotometer
      Integrating sphere attachment
    • Calibrated reference standards for transmittance and reflectance
    • Sample holder or mounting stage
    • Solar-simulated light source covering the terrestrial spectrum
    • Data acquisition and analysis software

    Results and Deliverables

    • Solar energy transmittance (%) of the test specimen
    • Solar energy reflectance (%) of the test specimen
    • Average values over the specified terrestrial solar spectrum
    • Individual spectral contributions, if reported
    • Test conditions (solar spectrum, angle of incidence, temperature)
    • Specimen identification and thickness
    • Observations on surface condition or anomalies during testing

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