The FPD-IG-175 fast optical detector is designed for visualizing and measuring the temporal characteristics of laser beams in the spectral range from 900 to 1700 nm. It has an InGaAs PIN photodiode and is used to convert optical signals into electrical signals which are then measured with third party measurement instrumentation such as oscilloscopes or spectrum analyzers for measurement. The FPD-IG-175 has a rise time of 175 ps.
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fpd-ig-175-fast-optical-detector - Drawings
Additional drawings are not available for this product.
Specifications
Product Name
FPD-IG-175
Sensor Type
InGaAs
Rise Time/Fall Time
<175 ps
Spectral Range
900-1700 nm
Active Area Diameter
0.1 mm
Noise Equivalent Power
<0.03 pW/√Hz
Detector Area
0.0079 mm²
Wavelength of Peak Sensitivity
1600 nm
Responsivity at Peak Wavelength
1.1 A/W
Responsivity (Irradiance) at Peak Wavelength
4.3 x 10⁻³ V/(W/cm²)
Bias Voltage
6 VDC
Bias Voltage Source
Batteries
Bandwidth
>2 GHz
Dark Current
<2 nA
Maximum Average Power
10 mW
Mounting (Tapped Holes)
8-32 & M4
Output Connector
BNC
Accessory Thread
M20x1
Dimensions
54 x 34 x 40 mm (LxWxD)
CE Compliance
Yes
UKCA Compliance
Yes
China RoHS Compliance
Yes
Features
Pulse Characterization Sensor Overview
Using these Ophir fast photodetectors, you can see and measure the temporal characteristics of pulsed and CW laser beams.
Fast Photodiode Spectral Responsivity
Responsivity is defined as the produced photocurrent (in Amperes) per Watt of incident radiation. It is a function of wavelength. Hence, the spectral response of the photodiode should be as high as possible at the wavelength of the laser to be measured. The spectral responsivities of the FPD series are shown in the figure. Ophir offers several fast photodiodes models with Silicon photodiodes having spectral response from 320 nm to 1100 nm, UV enhanced Silicon with extended response from 193 nm to 1100 nm, and InGaAs photodiodes which are sensitive from 900 nm to 1700 nm.
Pulse energy can be measured directly using one of Ophir's calibrated energy sensors. Another way is to use a calibrated power sensor and calculate the pulse energy using:
Pulse energy [J] = average power [W] / pulse rate [pulses per second]
Temporal sensors provide a signal that is proportional to the instantaneous power output of the laser. When viewing the pulse waveform on an oscilloscope, the integrated area under the curve is proportional to the total pulse energy.
Calibrated power sensorsmeasure the average power of CW and pulsed laser beams. The sensor is connected to an Ophir Meter or PC Interface. Power sensors are optimized for low noise and linear response in order to maximize power measurement accuracy. The measured laser beam must be smaller than the sensor's aperture in order to obtain an accurate power measurement. Temporal sensors are optimized for high speed response in order to reproduce pulse temporal characteristics with high fidelity. A temporal sensor is usually smaller than the laser beam size and samples a portion of the beam. The temporal sensor is connected to a scope or spectrum analyzer to display temporal characteristics of pulsed lasers.
There are a number of options, depending on the purpose.
In many cases, the simplest solution could be to make use of the analog output of the meter – that gives a voltage signal proportional to the actual reading (it is in fact just a D/A translation of what is being displayed), so it represents a fully calibrated reading. The full scale value is a function of the meter being used and the power range it is on.
) simply takes the raw output from the detector element and sends it to the scope. It bypasses the sensor's EEROM which contains the calibration data, so it essentially turns the sensor into an uncalibrated "dumb" analog sensor. It should be noted, though, that in some cases we could be talking about a signal to the scope that may be low, perhaps even near the noise level of the scope, which limits the usefulness of this method at low powers.
If the need is to see the pulse width – the temporal profile – the solution (assuming applicable specs) is to use an approprinte temporal sensor connected to a scope. You can point it anywhere where it will catch some backscatter from your laser, and you'll see the pulse temporal form as it really is.
Admittedly a unit such as “√ Hz” is not very intuitive. In general: Noise Equivalent Power (NEP) is defined as the signal power that gives a signal-to-noise ratio of 1 in a one-hertz output bandwidth. Taking the bandwidth of the measurement into account is where the “square root of Hz” comes in. The noise spectrum typically has a relatively flat response, and the noise level changes with the square root of the frequency range. For example, if the frequency range doubles, the noise component increases by √2 (1.414). In detector datasheets, the bandwidth is typically normalized to 1 Hz (which is usually far below the detection bandwidth), to allow detectors with different bandwidth specifications to be directly compared.
With a temporal detector you can measure the rise time, fall time, pulse duration and pulse frequency. Many laser applications use pulsed laser, for example medical lasers, LIDARs, and high power fiber laser for metal processing to name a few. The parameters of the laser pulses are critical for the performance of the application.
Pulse energy can be measured directly using one of Ophir's calibrated energy sensors. Another way is to use a calibrated power sensor and calculate the pulse energy using:
Pulse energy [J] = average power [W] / pulse rate [pulses per second]
Temporal sensors provide a signal that is proportional to the instantaneous power output of the laser. When viewing the pulse waveform on an oscilloscope, the integrated area under the curve is proportional to the total pulse energy.
Calibrated power sensorsmeasure the average power of CW and pulsed laser beams. The sensor is connected to an Ophir Meter or PC Interface. Power sensors are optimized for low noise and linear response in order to maximize power measurement accuracy. The measured laser beam must be smaller than the sensor's aperture in order to obtain an accurate power measurement. Temporal sensors are optimized for high speed response in order to reproduce pulse temporal characteristics with high fidelity. A temporal sensor is usually smaller than the laser beam size and samples a portion of the beam. The temporal sensor is connected to a scope or spectrum analyzer to display temporal characteristics of pulsed lasers.
There are a number of options, depending on the purpose.
In many cases, the simplest solution could be to make use of the analog output of the meter – that gives a voltage signal proportional to the actual reading (it is in fact just a D/A translation of what is being displayed), so it represents a fully calibrated reading. The full scale value is a function of the meter being used and the power range it is on.
) simply takes the raw output from the detector element and sends it to the scope. It bypasses the sensor's EEROM which contains the calibration data, so it essentially turns the sensor into an uncalibrated "dumb" analog sensor. It should be noted, though, that in some cases we could be talking about a signal to the scope that may be low, perhaps even near the noise level of the scope, which limits the usefulness of this method at low powers.
If the need is to see the pulse width – the temporal profile – the solution (assuming applicable specs) is to use an approprinte temporal sensor connected to a scope. You can point it anywhere where it will catch some backscatter from your laser, and you'll see the pulse temporal form as it really is.
Admittedly a unit such as “√ Hz” is not very intuitive. In general: Noise Equivalent Power (NEP) is defined as the signal power that gives a signal-to-noise ratio of 1 in a one-hertz output bandwidth. Taking the bandwidth of the measurement into account is where the “square root of Hz” comes in. The noise spectrum typically has a relatively flat response, and the noise level changes with the square root of the frequency range. For example, if the frequency range doubles, the noise component increases by √2 (1.414). In detector datasheets, the bandwidth is typically normalized to 1 Hz (which is usually far below the detection bandwidth), to allow detectors with different bandwidth specifications to be directly compared.
With a temporal detector you can measure the rise time, fall time, pulse duration and pulse frequency. Many laser applications use pulsed laser, for example medical lasers, LIDARs, and high power fiber laser for metal processing to name a few. The parameters of the laser pulses are critical for the performance of the application.
For mounting FPD sensor series (except FPS-1) to North Pole post of IS6 series.
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Extended Warranty for Sensor
Customers that purchase the above items also consider the following items. Ophir-Spiricon meters and sensors include a standard manufacturers warranty for one year. Add a one year Extended Warranty to your meter or sensor, which includes one recalibration.
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