The ultrafast PIN photodiodes have certain advantages over vacuum
photodiodes. Besides the compact size and low-voltage power supply, they
feature higher sensitivity, which is typically two orders of magnitude
larger in the near infrared as compared to vacuum photodiodes.
Because
of the extremely low dark current, the built-in high-power battery provides
trouble-free operation for UP TO FIVE YEARS*! In combination with our
ultrafast low-noise amplifiers (1 GHz bandwidth) the UPD-type
photodetectors are an inexpensive alternative to the avalanche devices.
Our UV-extended version is the only commercial photodiode that covers the
spectral range from 190 nm to 1100 nm and has risetime below 200 ps.
* UPD-300-IR, UPD-500 and monitoring of lasers with repetition rate >100 Hz require
external power supply!
EXAMPLE: UPD-200-UD-L
ultrafast photodetector with 200 ps rise time,
spectral range extended to UV, with diffusor,
for low rep. rate laser pulses < 100 Hz
ORDERING INFORMATION:
A PRACTICAL HINT!
In order to evaluate the performance of a
high-speed photodetector, you do not need a
short pulse laser source at all. Just take a
small He-Ne laser and focus the light on the
sensitive area of the PIN photodiode. You
will observe a signal modulated with very
high frequency due to the
. In the figure on the right, the
beating frequency f=c/2L (c -speed of light,
L - laser cavity length) is 1.5 Gigahertz!
Since this frequency is well above the
specified 1 GHz oscilloscope bandwidth,
the modulation depth in the figure is 25%
only.
longitudinal mode
beating
LONGITUDINAL MODE
BEATING OF A He-Ne LASER AS
DETECTED BY UPD-200-SP
PHOTODIODE
UPD-XXX-XX-X
Ultrafast photo detector
Rise time (picoseconds) Window type: P=Polished
D=Diffusor
Spectral range: U=Uv
S=visible
IR=Infrared
H=High rep. rate >100 Hz
L=Low rep. rate <100 Hz
ALPHALAS GmbH
Hannah-Vogt-Str. 1, D-37085 Göttingen, Germany
Tel.: +49-551-7706147, Fax: +49-551-7706146, E-mail: sales@alphalas.com, Web-Site: www.alphalas.com
ALPHALAS GmbH