Award-winning SolsTiS is a next generation continuous-wave Ti:Sapphire laser designed to meet the needs of pioneering scientists looking for high performance, ease of use, system flexibility and reliability. This fully-automated, compact system features a completely sealed, alignment-free cavity with hands-free operation, an unprecedented tuning range, unrivalled power, and the ultimate narrow linewidth, low-noise output. SolsTiS PI has an output power of >5 W, linewidths <100 kHz and amplitude noise of <0.075 %. Fully-integrated accessories such as beam pick-off and fiber coupling are available.
Continuous tuning from 700 - 1000 nm with a single optics set. Optional integrated frequency conversion modules can further extend this to cover 210 nm – 4 μm.
Ultra-narrow linewidths of <100 kHz absolute linewidth, with options to achieve Hertz level linewidth via an external, ultra-stable reference. Overall, SolsTiS is the quietest and most stable TiS laser available with free running linewidths close to 100 kHz.
Custom, low-loss optics in the laser ring resonator enable output power levels >5 W. There is no compromise from having a single device covering 300 nm, and exceptional power levels are found at the edges of the tuning range. High powers of >2.5 W are possible in SHG.
Continuous, single-mode, high-resolution scans over >25 GHz, up to 300 nm (with TeraScan option). Automatically stitch together consecutive segments to achieve high-resolution scans over >100 nm with high repeatability and linearity.
Smallest laser in its class. A sealed resonator eliminates dust contamination and enables robust, reliable performance. Materials minimise effects from vibrations and thermal variations, resulting in a stable, low-frequency drift laser. Anti-humidity system and purge ports allow trouble-free operation across atmospheric absorptions.
Fully-automated with wavelength tuning and locking via a web interface or published set of TCP/IP controls. Option to use third-party applications such as LabVIEW and MATLAB. Resonator elements are also accessible through external voltage inputs for active feedback.
Ultra-stable output with relative intensity noise 0.075 % RMS with exceptional stability on longer timescales. Automatic locking of cavity elements allows continuous running over long time durations with no interruptions.
Integrated extension modules are available to extend the tuning range from 210 nm to 4000 nm. These feature interlocking base plates and connecting lens tubes that enclose any beam paths not part of the final output. Beam pick off and fiber launch modules available.
The pump source Equinox, is a single-frequency CW 532 nm laser and is inherently stable, low-noise, naturally compact, robust and fully-automated. A linewidth <1 MHz makes it one of the narrowest linewidth lasers in its class.
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 world's first fully-automated, self-aligning, sealed, high power SHG cavity capable of rapid and precise, broad wavelength tuning and scanning in the UV and Visible up to 150nm.
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A compact frequency quadrupling module that extends the range of SolsTiS output wavelengths to produce narrow linewidth, tunable output in the ultraviolet.
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An external mixing module that offers fully automated tuning in the visible and IR with further extension options into the UV.
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Advanced automated laser system featuring a sealed high-power SHG cavity and frequency mixing module capable of precise wavelength tuning and reapid scanning across the visible, near-ultraviolet and near-infrared regions.
VIEW PRODUCTOr if you’d prefer to speak to someone in person, please phone +44 (0)1483 685 170
Phone +44 (0)141 945 0500
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