SOLSTIS ECD-X

  • CW
  • Tunable
  • UV
  • Visible

UV & VISIBLE SHG CAVITY

  • 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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The external cavity doubler SolsTiS ECD-X is an extension for SolsTiS. It extends the range of output wavelengths via frequency doubling in a resonant cavity with optimised conversion efficiency to generate high power output from 350-525 nm with a suite of crystals and a single optics set. Automatic, stable lock to SolsTiS is achieved with Hansch-Couillard locking. ECD-X automatically follows SolsTiS frequency scans to deliver >40 GHz of mode hope free tuning across the doubled wavelengths.

FEATURES


HIGHLY EFFICIENT

Highly efficient resonant doubling of CW input light with up to 50% conversion efficiency for higher powers and typically achieves 40% efficiency with just 1 W of fundamental power.

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.

BROAD WAVELENGTH COVERAGE

Interchangeable mounted crystal packages are available
for different wavelengths. A crystal covers more than 20 nm at any one time and it’s easy to interchange these crystals for extended coverage.

EXCELLENT BEAM QUALITY

SolsTiS ECD-X features exceptional beam conditioning optics <1.1 M2, which is helpful for using fiber launch.

OPTOMECHANICAL STABILITY

It’s the only doubling cavity system built on an Invar baseplate to provide maximum stability.

LOW INTERNAL HUMIDITY

Desiccant cavity reduces internal humidity with no requirement for purging.

SINGLE OPTICS SET

No need to change optics (internal or external) - single optics set for Ti:Sa fundamental range.

SPECIFICATIONS

Doubling Efficiency 6% for fundamental power 100-300 mW
10% for fundamental power 300-600 mW
15% for fundamental power 600-1000 mW
22% for fundamental power >1 W
Continuous Scan Range >40 GHz
Relative Intensity Noise <0.5 %
Beam Quality TEM00 M2 <1.2
Tuning Range 700 - 1000 nm
Fundamental Wavelength 700 nm, 800 nm, 900 nm
Typical Tuning Range +/- 15, +/- 25, +/-30
Operating temperature range16-30
Maximum relative humidity80% non-condensing, up to 30
Ice Bloc controller dimensions 34 cm x Half Rack x 2U, LxWxH
Laboratory requirements Mount on optical table with air free of dust
(Laminar airflow box recommended)

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-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
  • UV
  • visible
  • IR

SOLSTIS EMM

The SolsTiS External Mixing Module provides fully automated tuning in the visible (500-680 nm) and IR (1.1-4.5 µm) with further extension options into the UV (250-350 nm).

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

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