Collimation
MGL-W-556A: Collimation benefits from a stable, focusable source. 556 nm emission fixes the compatible coatings and detector response, while the listed beam characteristic (Near TEM00) informs waist size and propagation.
Power stability, linewidth, beam quality
MGL-W-556A is a 556 nm CW laser. Used for collimation, laser medical treatment, scientific experiment, optical instrument. Fan cooling and heat sink. Key specifications: output / average power 800~3000 mW, operating mode CW, power stability (rms, 4 hours ± 3°c) <5%, <3%, (<2% optional). View specifications, datasheet and enquiry options from Precisometer.
Specifications
19 specification rows
| Output / average power | 800~3000 mW |
|---|---|
| Beam / notes | Fan cooling and heat sink |
| Operating mode | CW |
| Power Stability (rms, 4 hours ± 3°C) | <5%, <3%, (<2% optional) |
| Transverse mode | Near TEM00 |
| M2 | 3-6 |
| Beam divergence, full angle (mrad) | <1.5 |
| Warm-up time (minutes) | <10 |
| Pointing Stability Over Temperature (urad/°C) | <20 |
| Polarization ratio | >50:1(100:1 optional), Horizontal(Vertical optional) |
| Operating temperature (°C) | 10-35 |
| Power supply (100-240VAC) | PSU-W-LED |
| Expected lifetime (hours) | >10000 |
| Wavelength (nm) | 556±1 |
| M² | 3-6 |
| Beam diameter at the aperture (1/e2, mm) | ~4.0 |
| Pointing Stability(urad) (over 2 hours after warm-up and ±3°C) | <50 |
| Beam height from base plate (mm) | 80 |
| Modulation option | DC-1kHz, 1kHz-10kHz, 10kHz-30kHz optional; TTL and Analog optional |
Application context
Applications named on this model’s datasheet, expanded with the model’s optical specifications.
MGL-W-556A: Collimation benefits from a stable, focusable source. 556 nm emission fixes the compatible coatings and detector response, while the listed beam characteristic (Near TEM00) informs waist size and propagation.
MGL-W-556A: 556 nm emission determines compatible optics, coatings and detectors for Laser medical treatment. The catalogued beam parameter (Near TEM00) helps predict how the source will focus and propagate through the instrument.
MGL-W-556A: 556 nm emission determines compatible optics, coatings and detectors for Scientific experiment. The catalogued beam parameter (Near TEM00) helps predict how the source will focus and propagate through the instrument.
MGL-W-556A: 556 nm emission determines compatible optics, coatings and detectors for Optical instrument. The catalogued beam parameter (Near TEM00) helps predict how the source will focus and propagate through the instrument.
System integration
Use these checks to connect MGL-W-556A to the surrounding optical, mechanical and control system. Every value shown is taken from this model's own specification record.
Technical FAQ
Operating temperature (°C): 10-35. Provide the stated cooling method and keep the laser-head base thermally coupled; temperature drift moves wavelength, output power and beam pointing.
Transverse mode: Near TEM00 · M2: 3-6. Size the downstream optics from the stated beam diameter and divergence rather than from the aperture of the housing, and confirm the polarisation state before specifying isolators or polarising optics.
Share wavelength, operating mode, output power or pulse energy, linewidth or pulse width, delivery, control, and safety requirements and we will qualify the matching configuration and lead time.
Model selection
Compare MGL-W-556A with the closest available models in the CW Lasers family. Confirm option-dependent values on the final configuration before ordering.
| Selection parameter | MGL-W-556A (current) | MLL-FN-556 | MGL-U-556 |
|---|---|---|---|
| Wavelength | 556 nm | 556 nm | 556 nm |
| Optical power / pulse energy | 800~3000 mW | 1~200 mW | 1~200 mW |
| Operating mode / pulse width | CW | CW | Confirm for this model |
| Beam quality | Near TEM00 | TEM00 | Confirm for this model |
Compare the MGL-W-556A with nearby cw lasers across the wavelength range.
Choosing a laser
Which specifications decide the experiment, and which ones cost money without changing the result.
PhotonicsLinewidth, spectral width, RIN, M², and coherence length answer five different questions. Translate each into the units your experiment is designed in — and learn which ones not to pay for.
Open guide
Optical trappingWhy wavelength is decided by photodamage, focal heating, and detector bandwidth rather than trapping force — and what laser noise costs you in piconewtons.
Open guide
Confocal microscopyConnect fluorophores, pinhole size, Airy units, spatial sampling, scan timing, modulation, and power after the fiber in one practical design workflow.
Open guide