LASER LINE TUNABLE FILTER

  • Efficiency up to 60%
  • High out-of-band rejection
  • Wide tuning range
  • Free-space or fiber coupled
  • User-friendly control software
Quotation
SPACE & ASTRONOMY

SPACE & ASTRONOMY

Finding a light-source for testing a coronagraph is challenging. Lasers are strongly collimated and many types of near-IR lasers would be powerful enough, but, other than Photon etc’s Tunable Laser Source, none is tunable over a very large wavelength domain.

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THIN FILMS

THIN FILMS

Magneto-optical (MO) effects are used either as tools for probing the magnetization reversal characteristics of a wide range of sample types, or as an effective way to modify the polarization of light via induced magnetization state in samples. In transparent samples, the Faraday effect, along with other MO effects such as Kerr measurements, provide a non-destructive probe for in-situ measurements of samples, such as thin films.

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Spectral Window 400 to 1000 nm
Bandwidth (FWHM) 2.5 nm
Pointing Stability < 1 mm lateral displacement @ 1m from filter
Peak Transmission up to 60%
Grating Damage Threshold > 100 kW/cm2 average power
  > 5 GW/cm2 peak power @ 1064 nm, 8 ns
Aperture Diameter ≤ 5 mm
Dimensions (L x W x H) 9'' x 6.3'' x 6.7''
  23 cm x 16 cm x 17 cm
Operating Temperature 10 to 40°C
Storage Temperature 5 to 50°C
Software PHySpecTM included
Computer Connection USB 2.0 (compatible 1.1)
Power Supply 100 - 240 V, 50 - 60 Hz
Wavelength Relative Resolution FWHM/8
Options Free-space/Fibered Output
  Order Filter
  Calibration Module
  Shutter
  FWHM < 0.4 nm