5–30 W at 532 nm
Match absorbed pump power to the Ti:Sapphire cavity.
Control with precision · Quantum & coherent research
Ti:Sapphire pumping
Feed a tunable ultrafast source with a quiet, high-quality green pump.
Application focus5–30 W at 532 nm
Low M² beam
Good mode quality supports efficient cavity overlap.
Low noise & drift
Pump fluctuations transfer into ultrafast output.
Why the source matters
Ti:Sapphire pumping is sensitive to pump stability, low noise, TEM00 beam quality, and thermal management.
The correct source is defined at the sample or process—not at the laser aperture. Wavelength and operating mode set the interaction; stability, delivery, timing, and control determine whether it stays useful in the complete system.
Light in532 nm, 5-30 W class
InteractionDrive a transition
Result5–30 W at 532 nm
Application workflow
Design from the result backward.
Three decisions turn the application into a practical source specification.
Start with the Ti:Sa cavity
Capture crystal, cavity geometry, absorbed power target, pump spot, and tuning goals.
Match the pump mode
Specify output power, beam diameter, M², polarization, pointing, and alignment height.
Plan heat and utilities
Confirm cooling, room temperature, electrical service, footprint, and warm-up behavior.
Selection guide
Match the architecture to the experiment.
These are starting architectures. Precisometer qualifies the final wavelength, output, delivery, control, and integration package against your setup.
- Wavelength band
- 532 nm, 5-30 W class
- Operating mode
- CW DPSS pump
Research oscillator pump
Prioritize quiet CW output, TEM00 beam quality, and easy power adjustment.
Higher-power amplifier pump
Include cooling, long-term stability, and facility requirements.
Retrofit
Match beam height, direction, footprint, cooling, and electrical interface.
Ready to specify
Bring us the application—not a guessed model number.
Ask for Ti:Sa cavity, pump power, beam diameter, M2 target, noise target, cooling constraints, and available mains power.
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