Power stability, linewidth, beam quality
MLL-III-1060-SM is a 1060 nm CW laser. Used for medical imaging, flow cytometry, dna sequencing. SM Fiber output laser. Key specifications: output / average power 1~500 mW, power stability (rms, 4 hours ± 3°c) <2%, <1%, <0.5%, fiber type SM fiber, PM fiber optional. View specifications, datasheet and enquiry options from Precisometer.
Specifications
21 specification rows
| Output / average power | 1~500 mW |
|---|---|
| Beam / notes | SM Fiber output laser |
| Power stability (rms, 4 hours ± 3°C) | <2%, <1%, <0.5% |
| Fiber type | SM fiber, PM fiber optional |
| Fiber connector | FC/PC, FC/APC optional |
| Fiber jacket | Metal, PVC optional |
| Power supply (100-240VAC) | PSU-III-FDA/PSU-III-LED/PSU-A-D/PSU-III-OEM |
| Modulation option | DC-1kHz, 1kHz-10kHz, 10kHz-30kHz, 30kHz-100kHz optional; TTL and Analog optional |
| Central wavelength (nm) | 1060±10 |
| Operating mode | CW |
| Output power after fiber (mW) | 1-10 |
| Noise of amplitude (rms, 20Hz-20MHz) | <1%, <0.5% |
| Fiber Core diameter | 4-9μm, 0.12NA |
| Fiber length | 1m |
| Transverse mode | TEM00 |
| Ellipticity | >0.95 |
| M2 after fiber | ~1.1 |
| Warm-up time (minutes) | <5 |
| Cooled method | Conduction |
| Operating temperature (°C) | 10-35 |
| Expected lifetime (hours) | >10000 |
Application context
Applications named on this model’s datasheet, expanded with the model’s optical specifications.
MLL-III-1060-SM: 1060 nm emission can be matched to the absorption or excitation band used in Medical imaging. The stated stability or noise figure (<2%, <1%, <0.5%) helps keep measured intensity changes attributable to the sample rather than source drift.
MLL-III-1060-SM: 1060 nm emission can be matched to the absorption or excitation band used in Flow cytometry. The stated stability or noise figure (<2%, <1%, <0.5%) helps keep measured intensity changes attributable to the sample rather than source drift.
MLL-III-1060-SM: 1060 nm emission can be matched to the absorption or excitation band used in DNA sequencing. The stated stability or noise figure (<2%, <1%, <0.5%) helps keep measured intensity changes attributable to the sample rather than source drift.
System integration
Use these checks to connect MLL-III-1060-SM to the surrounding optical, mechanical and control system. Every value shown is taken from this model's own specification record.
Technical FAQ
Fiber type: SM fiber, PM fiber optional · Fiber connector: FC/PC, FC/APC optional. Match the listed connector and fiber mode exactly; SMA905, FC/PC and FC/APC are not interchangeable, and a single-mode launch requires mode-field as well as numerical-aperture matching.
Cooled method: Conduction · 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: TEM00 · M2 after fiber: ~1.1. 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 MLL-III-1060-SM with the closest available models in the CW Lasers family. Confirm option-dependent values on the final configuration before ordering.
| Selection parameter | MLL-III-1060-SM (current) | MDL-1060(FC) | FC-1060 |
|---|---|---|---|
| Wavelength | 1060 nm | 1060 nm | 1060 nm |
| Optical power / pulse energy | 1~500 mW | 1~2000 mW | 1~20 W |
| Operating mode / pulse width | CW | CW | Confirm for this model |
| Beam quality | TEM00 | Multimode | Confirm for this model |
Compare the MLL-III-1060-SM 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