The SolsTiS External Mixing Module (SolsTiS EMM) provides fully automated tuning in the visible (480-670 nm) and IR (1.1-4.5 µm) with further extensions options into the UV (300-350 nm). It delivers high stability sum and difference frequency mixing of SolsTiS wavelengths with other single frequency sources, primarily via high efficiency single pass mixing in PPLN. This all-solid state solution for wavelength coverage supersedes dye lasers, removing the hazards and instabilities associated with this toxic gain material. SolsTiS EMM delivers unparalleled performance and reliability, enabling you to automatically tune and scan over a broad wavelength range.
SolsTiS EMM is the natural successor to out-dated and hazardous dye laser technology, offering a completely automated and low noise alternative.
Solid-state solution for wavelength tuning in the visible – no toxic dyes.
No power degradation over time.
No need to change optics (internal or external) – a single optics set for the Ti:Sapphire fundamental range.
An easy to use web interface controls fine wavelength tuning (automatic tracking of fundamental frequency scans) and locking. Alternatively, you can use a published set of TCP/IP controls for third party applications such as LabVIEW and MATLAB.
SolsTiS EMM-532
SolsTiS EMM-1550 and EMM-1950
| Model | Wavelength | Power | ||
|---|---|---|---|---|
| EMM-1550 | 500-540 nm 540–580 nm 580-600 nm |
>0.5 W >0.4 W >0.2 W |
||
| EMM-1950 | 525-600 nm 515-525 nm, 600-650 nm 650-661 nm |
>100 mW >50 mW >25 mW |
||
| Tuning range | ||||
| Model | Optics | Crystals | ||
| EMM-1550 | 500-600 nm | 500-533 nm 527-565 nm 533-600 nm |
||
| EMM-1950 | 515-661 nm | 515-582 nm 582-661 nm |
||
| Scan range | > 25 GHz | |||
| Intensity noise | < 0.25% RMS integrating over range, 10 kHz-10 MHz |
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M Squared’s lasers are both remarkable in their performance and beautiful in their design. They have enabled my Group’s research over the last decade and will continue to transform many areas of science and technology.
Professor Miles Padgett
University of Glasgow
Professor Miles Padgett holds the position of Professor and Kelvin Chair of Natural Philosophy at the University of Glasgow’s School of Physics and Astronomy.
*The Center for Ultracold Atoms (CUA) comprises a community of scientists from Harvard University and the Massachusetts Institute of Technology (MIT). The CUA is supported by the National Science Foundation (NSF).
M Squared’s’ SolsTiS laser platform transformed our quantum optics experiments, helping to produce several documented breakthroughs. In fact, we were so impressed with its performance and versatility that we went on to purchase another four.
Professor Charles Adams
University of Durham
Professor Charles Adams works in the Department of Physics at the University of Durham, is a Member of the Centre for Atomic and Molecular Physics and is Director of the Joint Quantum Centre.
A range of extensions are available to enhance the wavelength coverage of the system, helping you to explore new regions.
The award-winning SolsTiS is a step-change in continuous-wave Ti:Sapphire laser technology - compact, ultra-narrow linewidth, fully automated and widely tunable.
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A compact frequency conversion module that extends the range of SolsTiS output wavelengths via frequency doubling in a resonant cavity with optimised conversion efficiency.
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This SolsTiS extension adds a frequency quadrupling feature to SolsTiS, producing a narrow linewidth, tunable output in the ultraviolet wavelengths.
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Equinox is a single frequency CW 532 nm laser (up to 18W). It’s inherently stable, low noise, narrow linewidth and naturally compact, robust and fully-automated.
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