LimsPulse
SPF analyser · Calibration procedure

Wavelength and transmittance verification

Checks that the SPF analyser reads wavelengths correctly with a holmium oxide filter and reads transmittance correctly with certified neutral-density (or UV-absorbing) filters, then confirms the whole system with a reference sunscreen.

Illustration of SPF analyser
PURPOSE

Why this is checked

SPF and UVA-PF are calculated by weighting transmittance at each wavelength with steep action spectra. A wavelength shift of a nanometre or two in the UVB region, or a small transmittance error where the film lets little light through, changes the result noticeably. This check proves both axes of the spectrum are right before results are reported.

Frequency

Typically every 6–12 months, after a lamp change, repair or relocation, and whenever the reference sunscreen trends out of range, as defined in your SOP. A quick filter check before each series is good practice.

Learn how the SPF analyser works
YOU WILL NEED

Standards & tools

  • Holmium oxide glass wavelength filter with a traceable certificate (peaks in the UV such as near 279, 287, 334 and 361 nm)
  • Certified neutral-density or UV transmittance filters covering low to medium transmittance (for example about 10%, 30% and 50% T)
  • Clean blank PMMA plate (glycerine-coated, as for routine blanks)
  • Reference sunscreen with an expected value range, as given by the method (for example the ISO 24443 reference product)
BEFORE YOU START

Prerequisites

  • Lamp warmed up for the time stated in the manual
  • Filters clean, undamaged and within certification date
  • Room at normal laboratory temperature, instrument free from vibration
PROCEDURE

Step by step

  1. 1Run a baseline (100% T) with an empty beam or blank plate as the manual describes.
  2. 2Insert the holmium oxide filter and scan 270–400 nm in 1 nm steps (or finer if available).
  3. 3Find the wavelength of each certified absorbance peak and record it.
  4. 4Calculate the error for each peak (measured − certified).
  5. 5Insert each transmittance filter in turn and record %T at the certified wavelengths (for example 300, 350 and 380 nm).
  6. 6Calculate the transmittance error for each filter and wavelength.
  7. 7Apply a reference sunscreen to plates as per the routine method and measure it; compare with its expected range.
  8. 8Record all results, filter serial numbers and certificate dates.
RECORD

Example observation table

CheckCertified valueMeasuredErrorTolerance (typical)Result
Holmium peak 1279.3 nm279.6 nm+0.3 nm± 1 nmPass
Holmium peak 2287.6 nm287.4 nm−0.2 nm± 1 nmPass
Holmium peak 3333.8 nm334.1 nm+0.3 nm± 1 nmPass
Holmium peak 4360.8 nm361.2 nm+0.4 nm± 1 nmPass
Filter A at 300 nm10.2 %T10.4 %T+0.2 %TAs per SOP / manufacturerPass
Filter B at 350 nm30.5 %T30.1 %T−0.4 %TAs per SOP / manufacturerPass
Filter C at 380 nm50.1 %T50.6 %T+0.5 %TAs per SOP / manufacturerPass
CALCULATION

How to calculate the result

Formula
Wavelength error = λ measured − λ certified; Transmittance error = %T measured − %T certified (absolute)
Worked example
  1. 1

    Holmium peak 4: 361.2 − 360.8 = +0.4 nm, within ± 1 nm

  2. 2

    Filter B at 350 nm: 30.1 − 30.5 = −0.4 %T

  3. 3

    As absorbance, filter B reads −log₁₀(0.301) = 0.521 against a certified −log₁₀(0.305) = 0.516

ACCEPTANCE CRITERIA

Pass if

  • Wavelength accuracy typically within ± 1 nm of the certified peak values, or the manufacturer's specification
  • Transmittance accuracy within the manufacturer's specification or your SOP limit (often about ± 1–2 %T absolute in the working range)
  • Reference sunscreen within the expected range stated in the method
IF IT FAILS

What to do

  • Label the instrument out of use for reportable testing.
  • Clean the optics and filters and repeat once to rule out a handling error.
  • If still failing, call the service engineer for realignment or lamp replacement.
  • Re-verify after repair and assess any results reported since the last good check.
In LimsPulse · Calibration Management

LimsPulse schedules this calibration, records the result against limits, and blocks the instrument everywhere if it fails or goes overdue.

See how