LED, picosecond & calibration sources
Wavelength Calibration Lamps
Mercury and mercury–neon line sources for checking the wavelength scale of a spectrometer. Choose a calibration-lamp assembly to match the entrance slit and the emission lines required by the instrument.
Best suited to
Spectrometer wavelength calibration and verification with discrete reference emission lines.
Selecting a configuration
Match the lamp spectrum and mechanical interface to the spectrometer. LSH-HgNe-A fits motorised slit arrangements; LSH-HgNe-B fits manual slit arrangements.
Measurement & configuration
- Mercury emission lines cover UV and visible wavelength references.
- Mercury–neon assemblies extend the set of available reference lines.
- Source-specific lamp mounting for compatible spectrometer entrances.
Plan the signal path
- 1Reference emission lamp
- 2Spectrometer entrance
- 3Wavelength-scale verification
Specifications
| Mercury lines (nm) | 253.65, 312.57, 313.15, 313.18, 365.02, 404.66, 435.84, 546.07, 576.96, 579.07 |
|---|---|
| LSW-Hg lamp power | 3 W |
| LSW-Hg current | 10 mA |
| LSW-Hg starting voltage | 1500 V |
| LSH-HgNe-A interface | Motorised slit |
| LSH-HgNe-B interface | Manual slit |
Configuration note: These are wavelength-reference lamps. Calibrated spectral irradiance, radiant flux or traceable radiometric output is not claimed.
Configure LHM254 / LSH-HgNe-A / B
Send the wavelength interval, signal level, timing and sample requirements for your experiment.