SOLSTIS EMM

  • CW
  • Tunable
  • UV
  • visible
  • IR

UV & VISIBLE FREQUENCY MIXING MODULE

  • 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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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.

FEATURES


LOW AMPLITUDE NOISE

SolsTiS EMM is the natural successor to out-dated and hazardous dye laser technology, offering a completely automated and low noise alternative.

SAFE TO USE

Solid-state solution for wavelength tuning in the visible – no toxic dyes.

LONG TERM POWER STABILITY

No power degradation over time.

SINGLE OPTICS SET

No need to change optics (internal or external) – a single optics set for the Ti:Sapphire fundamental range.

EASY TO CONTROL

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.

SPECIFICATIONS

SolsTiS EMM-532

Conversion efficiency > 1% of the product of the input powers
Example specification Input 1: 2 W @ 822 nm

Sum frequency: > 100 mW @ 323 nm
Continuous scan range >25GHz
Tuning range
Optics Input 1: 670-1050 nm
Input 2:
532 nm
Sum frequency 300-350 nm
Crystals ± 5 nm at centre of operation
Frequency and intensity noise
Linewidth of laser at 532 nm DPSS: <5MHz
Intensity noise of laser at 532 nm DPSS: <0.2%RMS

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

TRUSTED BY THE WORLDS’ LEADING UNIVERSITIES
AND RESEARCH INSTITUTIONS

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.

SOLSTIS EXTENSIONS

A range of extensions are available to enhance the wavelength coverage of the system, helping you to explore new regions.

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  • CW
  • Tunable
  • NIR

SOLSTIS

The award-winning SolsTiS is a step-change in continuous-wave Ti:Sapphire laser technology - compact, ultra-narrow linewidth, fully automated and widely tunable.

VIEW PRODUCT
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  • CW
  • Tunable
  • UV

SOLSTIS ECD-X

A compact frequency conversion module that extends the range of SolsTiS output wavelengths via frequency doubling in a resonant cavity with optimised conversion efficiency.

VIEW PRODUCT
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  • CW
  • Tunable
  • UV

SOLSTIS ECD-X-Q

This SolsTiS extension adds a frequency quadrupling feature to SolsTiS, producing a narrow linewidth, tunable output in the ultraviolet wavelengths.

VIEW PRODUCT
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  • CW
  • Tunable

EQUINOX

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.

VIEW PRODUCT

GET IN TOUCH WITH OUR SPECIALISTS

Or if you’d prefer to speak to someone in person, please phone +44 (0)1483 685 170

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Phone +44 (0)141 945 0500

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Phone +1-617-401-2368

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