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Simple and compact autocorrelator for measuring the pulse duration of modelocked femtosecond lasers.
- Resolution 2 femtoseconds
- Operates across Ti:Sapphire tuning range
- Set-and-forget alignment
- Based on 2-photon autocorrelation in a GaAsP LED*
- Displays intensity or interferometric autocorrelation
- Insensitive to polarisation of laser
- Compact and portable
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Part No. |
E750 |
Price |
$8745 |
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Price includes shipping and handling fees |
Manufactured in the UK |
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The TIMEWARPTM autocorrelator is based on the proven Michelson interferometer configuration for splitting an incoming pulse train into two daughter trains which produce the autocorrelation signal when recombined on a detector. It is manufactured under exclusive license from the University of St. Andrews. A varying delay is provided by mounting one mirror on the central cone of a small loudspeaker driven at 18Hz.
The two pulse trains are recombined on an GaAsP LED* where 2 photon absorption occurs and the autocorrelation appears as an electrical signal. This technique has a number of significant advantages over conventional methods for measurement of Ultrafast pulses:
- No PMT / non-linear crystal combination required
- Simple to set up and align
- Compact - takes minimal space on table
- Insensitive to input polarisation
The Timewarp E750 autocorrelator consists of an optical head and a control unit plus external mains power supply. The optical head houses the scanning interferometer and fits directly onto an M4 post mount for quick and easy alignment to the laser being measured using an alignment jig that is included. All of the optics in this interferometer are reflective apart from the beamsplitter, which is very thin to reduce the effects of dispersion on the incoming pulse.
The path lengths in the two arms of the interferometer need to be equal and this can be adjusted via a recessed hex head screw in the side of the unit. Recessed adjustments are also provided for the fixed mirror tilt so that the two beams can be overlapped and recombined on the detector. The small size of the interferometer and high mechanical stability of the unit mean that only minor adjustments to the alignment will be necessary after installation in order to display an autocorrelation trace.
The Controller unit houses the drive circuitry for the loudspeaker which generates the scan in the interferometer plus the signal conditioning. Front panel controls are provided for adjustment of the amplitude of the scan and the phase of the signal fed into the oscilloscope. All connections are on the rear panel including 12VDC input, connection to the optical head (cable supplied), Trigger and Signal connections to the oscilloscope and the sync. input and output connectors for daisy-chaining two units together.
Specifications: |
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Wavelength Range |
700 - 1250 nm |
Pulse Duration Measurement Range |
<15 to 500 fs |
Optical Power Range |
2 < 8 mW Average Input Power |
Input Rep. Rate |
> 10MHz |
Resolution |
2 fs |
Scan Amplitude |
0 - 500 fs |
Scan Rate |
18 Hz |
Polarisation Dependence |
Polarisation Insensitive |
Non-linearity |
1 % |
Trigger Phase |
Variable +/- 90 degrees |
Damage Threshold |
200 mW |
Post Mounting |
M4 thread |
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Ancillaries |
Twin pinhole alignment jig included |
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Physical Dimensions |
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Optical Head |
120mm (W) x 65mm (H) x 125mm (D) |
Controller |
120mm (W) x 65mm (H) x 125mm (D) |
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Weight |
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Optical Head |
250 g |
Controller |
300g |
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Electrical |
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Operating Voltage |
110V / 230V |
Controller |
12V DC via supplied PSU |
Signal Output |
~ 200 mV |
Trigger
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Trigger signal generated internally - can be used to sync two units together |
Options and Accessories
Other operating wavelengths available

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Optical Head - Front Panel |
Optical Head - Rear Panel |

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Controller - Front Panel |
Controller - Rear Pane |
* Patent No USA 6195167
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