The overall task of the optical
receiver is to extract the information that has been placed on the modulated light carrier
by the distant transmitter and restores the information to its original form. The typical
through-the-air communications receiver can be broken down into five separate sections.
These are: light collector (lens), light detector (PIN), current to voltage converter,
signal amplifier and pulse discriminator. There may also be additional circuits depending
on the kind of the signal being received. As an example, a receiver that is extracting
voice information will need a frequency to voltage converter and an audio amplifier to
reproduce the original voice signal. Computer data receivers will also need some decoding
circuits that would configure the transmitted serial data bits into 8 bit words. However,
this section will concentrate on the circuits needed for processing voice information.
Volume II of this book will contain additional circuits for digital data receivers.
For long-range applications it is
essential to collect the weak modulated light from the distant transmitter with a glass or
plastic lens and focus it onto a silicon PIN photodiode. Although mirrors could also be
used to collect the light, glass or plastic lenses are easier to use and cost less.
Plastic lenses measuring from a fraction of an inch to six inches are available. For a
system that demands a large lens, the flat "Fresnel" lens is much less expensive
than a solid lens. Forming special concentric bumps in a clear plastic sheet makes Fresnel
lenses. The bumps bend the light just as a conventional thick lens would. Fresnel lenses
are available with diameters of several feet.
For certain short-range
applications it may also be possible to use a naked light detector without any lens.
Distances up to several hundred feet are possible with systems that don't rely on lenses
at either the transmitter or the receiver. Lens-less systems are especially useful when
very wide acceptance angles are required. Many cordless IR stereo headsets use two or more
naked detectors to provide acceptance angles approaching 360 degrees.
The lens chosen should be
as large as possible but not too large. A lens that is too large can produce a half angle
acceptance angle that is too small. Acceptance angles less than about 0.3 degrees will
result in alignment difficulties. Building sway and atmospheric disturbances can cause
signal disruption with narrow acceptance angles. A rough rule-of-thumb might be that the
lens diameter should not be more than 100 times larger than diameter of the active area of
the PIN detector. Also, the receiver should never be positioned so sunlight could be
focused onto the light detector. Even a brief instant of focused sunlight will destroy the
sensor. A north/south alignment for the transmitter and the receiver will usually prevent
an optical system from going blind from focused sunlight.
|As discussed in the section on
light detectors, the silicon PIN photodiode is the recommended detector for most all
through-the-air communications. Such a detector works best when reversed biased. In the
reversed biased mode it becomes a diode that leaks current in response to the light
striking it. The current is directly proportional to the incident light power level (light
|When detecting light at its peak spectrum response
wavelength of 900 nanometers, the silicon PIN photodiode will leak about 0.5 micro amps of
current for each microwatt of light striking it. This relationship is independent to the
size of the detector. The PIN photodiode size should be chosen based on the required
frequency response and the desired acceptance angle with the lens being used. Large PIN
photodiodes will have slower response times than smaller devices. For example, 1 cm X 1 cm
diodes should not be used for modulation frequencies beyond 200KHz, while 2.5 mm X 2.5 mm
diodes will work beyond 50MHz. If a long range is desired, the largest photodiode possible
that will handle the modulation frequency should be used.
STRAY LIGHT FILTERS
|Some systems can benefit from the placement of an
optical filter between the lens and the photodiode. The filter can reduce the effects of
sunlight and some stray light from distant street lamps. Filters can be especially
effective if the light detector is going to be processing light from a diode laser. Since
laser light has a very narrow bandwidth, an optical band pass filter that perfectly
matches the laser light can make a light receiver nearly blind to stray sunlight.
|If light emitting diode light
sources are used, optical filters with a much broader bandwidth are needed. Such a filter
may be needed for some situations where man-made light is severe. Many electronically
controlled fluorescent and metal vapor lamps can produce unwanted modulated light that
could interfere with the light from the distant transmitter.
But, in all but a few rare
exceptions, band pass filters produce few overall improvements if the correct detector
circuit is used. Since no optical filter is perfectly transparent, the noise reduction
benefits of the filter usually do not out weigh the loss of light through the filter.
Also, if the detector is going to process mostly visible light, no optical filter should
CURRENT TO VOLTAGE
The current from the PIN detector
is usually converted to a voltage before the signal is amplified. The current to voltage
converter is perhaps the most important section of any optical receiver circuit. An
improperly designed circuit will often suffer from excessive noise associated with ambient
light focused onto the detector. Many published magazine circuits and even many
commercially made optical communications systems fall short of achievable goals from
poorly designed front-end circuits. Many of these circuits are greatly influenced by
ambient light and therefore suffer from poor sensitivity and shorter operating ranges when
used in bright light conditions. To get the most from your optical through-the-air system
you need to use the right front-end circuit.
High Impedance Detector Circuit
|One method that
is often shown in many published circuits, to convert the leakage current into a voltage,
is illustrated in figure 6a.
This simple "high
impedance" technique uses a resistor to develop a voltage proportional to the light
detector current. However, the circuit suffers from several weaknesses. If the resistance
of the high impedance circuit is too high, the leakage current, caused by ambient light,
could saturate the PIN diode, preventing the modulated signal from ever being detected.
Saturation occurs when the voltage drop across the resistor, from the photo diode leakage
current, approaches the voltage used to bias the PIN device. To prevent saturation, the
PIN must maintain a bias voltage of at least a few volts.
|Consider the following
example. Under certain bright background conditions a PIN photodiode leakage current of a
few milliamps may be possible. If a 12v bias voltage were used, the detector resistance
would have to be less than 10,000 ohms to avoid saturation. With a 10K resistor, the
conversion would then be about 10 millivolts for each microamp of PIN leakage current.
But, to extract the weak signal of interest that may be a million times weaker than the
ambient light level, the resistance should to be as high as possible to get the best
current to voltage conversion. These two needs conflict with each other in the high
impedance technique and will always yield a less than desirable compromise
In addition to a low current to voltage
conversion, there is also a frequency response penalty paid when using a simple high
impedance detector circuit. The capacitance of the PIN diode and the circuit wiring
capacitance all tend to act as frequency filters and will cause the circuit to have a
lower impedance when used with the high frequencies associated with light pulses.
Furthermore, the high impedance technique also does not discriminate between low or high
frequency light signals. Flickering streetlights, lightning flashes or even reflections
off distant car windshields could be picked up along with the weak signal of interest. The
high impedance circuit is therefore not recommended for long-range optical communications.
Transimpedance Amplifier Detector Circuit With
over the high impedance method is the "transimpedance amplifier" as shown in
|The resistor that converts
the current to a voltage is connected from the output to the input of an inverting
amplifier. The amplifier acts as a buffer and produces an output voltage proportional to
the photodiode current. The most important improvement the transimpedance amplifier
has over the simple high impedance circuit is its canceling effect of the circuit wiring
and diode capacitance. The effective lower capacitance allows the circuit to work at much
higher frequencies. However, as in the high impedance method, the circuit still uses a
fixed resistor to convert the current to a voltage and is thus prone to saturation and
interference from ambient light.
Detector Circuit With Inductor Feedback
A dramatic improvement of the
transimpedance amplifier with a resistor feedback load is shown in figure 6c. This
technique is borrowed from similar circuits used in radio receivers. The circuit replaces
the resistor with an inductor. A student in electronics may remember that an inductor will
pass DC unaffected but will exhibit a resistance effect or reactance to AC signals. The
higher the frequency of the AC signals the higher the reactance.
This reactance circuit is exactly
what is needed to help extract the sometimes small modulated AC light signal from the
large DC component caused by unmodulated ambient light. DC signals from ambient light will
yield a low current to voltage conversion while high frequency AC signals will experience
a high current to voltage conversion. With the right circuit, an AC vs. DC conversion
ratio of several million is possible. Such techniques are used throughout radio receiver
circuits to process weak signals
In addition, as the Q increases so does the
impedance of the LC circuit. Such high Q circuits can also be used in a
transimpedance amplifier designed for optical communications. To obtain the
highest possible overall impedance, the inductance value should be as large
as possible and the capacitance should be as small as possible. Since every
inductor contains some finite parallel capacitance within its assembly, the
highest practical impedance occurs when only the capacitance associated with
the inductor assembly is used to form the LC network.
|In radio, connecting a
capacitor in parallel with the inductor often produces high impedances and allowing the LC
tuned circuit to resonant at a specific frequency. Such a circuit can be very frequency
selective and can yield impedances of several mega ohms. The degree of rejection to
frequencies outside the center resonant frequency is defined as the "Q" of the
circuit. As figure 6d depicts, a high Q will produce a narrower acceptance band of
frequencies than lower Q circuits.
Self Resonance Frequencies
|You can calculate the equivalent parallel
capacitance of an inductor based on the published "self-resonance" frequency or
you can use a simple test circuit to actually measure the resonance frequency in PDF Figure 6e of a coil. Figure 6f lists the
characteristics of some typical coils.
Transimpedance Amplifier Detector Circuit with
|The use of a
LC tuned circuit in a transimpedance amplifier circuit does improve the current to voltage
conversion and does reject much of the signals associated with ambient light. But, high Q
circuits are prone to unwanted oscillations. As shown in figure 6g, to keep the circuit
from misbehaving, a resistor should be wired in parallel with the inductor. The effect of
the resistor is to lower the circuit's Q. For pulse stream applications with low duty
cycles (short pulses with lots of time between pulses), it is best to keep the Q near 1.
|A Q of one exists when the
reactance of the coil is equal to the parallel resistance at the desired frequency. If
higher Qs were used, with low duty cycle pulse streams, the transimpedance amplifier would
produce excessive ringing with each pulse and would be prone to self-oscillation.
|Figure 6h and 6i illustrate
what happens in a circuit with a low Q and high Q when processing single pulses. If higher
duty cycle pulse trains are being transmitted, higher Qs can be used. In near 50% duty
cycle transmission systems, Qs in excess of 50 are possible with a careful design. Table
6f lists the typical self-resonant frequency of some inductors. If you don't know the
self-resonant frequency of a coil you can use the schematic shown in PDF Figure 6e to measure it.
In low duty cycle light pulse applications, the inductor value
should be chosen based on the width of the light pulse being sent by the transmitter. The
self-resonant period (1/frequency) of the coil should equal 2W, where W is the width of
the light pulse. Since the circuit layout, the amplifier circuit and the PIN diode will
all add to the overall circuit capacitance, some experimentation will be necessary to
determine the best inductor value for the particular application. The equation 2pFL should
be used to calculate the value of the resistor wired in parallel to the inductor to limit
the Q to 1.
PDF Figure 6j
is an example of a complete transimpedance amplifier circuit with inductive feedback. The
amplifier circuit shown in PDF Figure 6jhas a
light power to voltage conversion of about 23 millivolts per milliwatt (assuming 50% PIN
conversion) when used with 1 microsecond light pulses. Such an amplifier should be able to
detect light pulses as weak as one nanowatt during dark nighttime conditions.
POST SIGNAL AMPLIFIER
As discussed above, the
transimpedance amplifier converts the PIN current to a voltage. However, it may be too
much to expect one amplifier stage to boost the signal of interest to a useful level.
Typically, one or more voltage amplifier stages after the front end circuit are needed.
Often the post amplifiers will include some additional signal filters so only the desired
signals are amplified, rejecting more of the undesired noise. A general purpose post
amplifier is shown in figure 6j. The circuit uses a quality operational amplifier
in conjunction with some filter circuits designed to process light pulses lasting about 1
micro second. The circuit boosts the signal by a factor of X20.
SIGNAL PULSE DISCRIMINATOR
Once the signal has been
sufficiently amplified and filtered, it often needs to be separated completely from any
background noise. Since most systems use pulse frequency modulation techniques to transmit
the information, the most common method to separate the signal from noise is with the use
of a voltage comparator. The comparator can produce an output signal that is thousands of
times higher in amplitude than the input signal. As an example, a properly designed
comparator circuit can produce a 5 volt peak to peak TTL logic output signal from a input
of only a few millivolts.
But, to insure that the comparator can faithfully
extract the signal of interest, the signal must be greater in amplitude than any noise by
a sizeable margin. For most applications, I recommend that the signal to noise ratio
exceed a factor of at least 10:1 (20db). Then, with a properly designed comparator
circuit, the comparator output would change state (toggle) only when a signal is present
and will not be effected by noise.
A complete signal
discriminator circuit is shown in PDF Figure 6k.
The circuit is designed so a positive input pulse needs to exceed a threshold voltage
before the comparator produces a negative output pulse. A variable resistor network allows
the threshold voltage to be adjustable. The adjustment thereby provides a means to set the
sensitivity of the circuit. The adjustment should be made under the worst case bright
background conditions so the noise produced by the bright background light does not toggle
FREQUENCY TO VOLTAGE
|If the light pulses being
transmitted are frequency modulated to carry the information, then the reverse must be
done to restore the original information. The pulse frequency must therefore be converted
back into the original amplitude changing signal. A simple but very effective frequency to
voltage converter circuit is shown in PDF Figure 6k. Each pulse from the pulse
discriminator circuit is converted into a well defined logic level pulse that lasts for a
specific time. As the frequency increases and decreases, the time between the pulses will
change. The changing frequency will therefore cause the average voltage level of the
signal produced by the converter to change by the same proportion. To remove the unwanted
carrier frequency from the desired modulation frequency, the output of the converter must
MODULATION FREQUENCY FILTER
A complete filter circuit is
shown in PDF Figure 6l. The circuit uses a
switched capacitor filter (SCF) integrated circuit from National Semiconductor. With the
values chosen, the circuit removes the majority of a 10KHz carrier signal, leaving the
wanted voice audio frequencies. The filter's cutoff frequency is set at about 3KHz that is
the minimum upper frequency needed for voice audio.
AUDIO POWER AMPLIFIER
The final circuit needed to
complete a voice grade light pulse receiver is an audio power amplifier. The circuit shown
in PDF Figure 6l. uses a single inexpensive LM386
IC. The circuit is designed to drive a pair of audio headphones. The variable resistor
shown is used to adjust the audio volume. Since the voice audio system described above
does not transmit stereo audio, the left and right headphones are wired in parallel so
both ears receive the same audio signal.
LIGHT RECEIVER NOISE
One of the most difficult
problems to overcome in an optical through the air communications system is ambient light.
Any stray sunlight or bright background light that is collected by the receiver optics and
focused onto the light detector will produce a large steady state DC level through the
detector circuit. Although much of the DC is ignored with the use of an inductive feedback
amplifier method in the front-end circuit, the large DC component in the light detector
will produce some unwanted broadband noise. The noise is very much like the background
static you may hear on an AM radio when tuning the dial between stations. As discussed in
the section on light detectors, the amount of noise produced by the detector is
The equation shown in figure 6m describes how
the detector noise varies with ambient light. The relationship follows a square root
function. That means if the ambient light level increases by a factor of four, the noise
produced at the detector only doubles. This characteristic both helps and hurts a light
receiver circuit, depending on whether the system is being used during the light of day or
during the dark of night. The equation predicts that for high ambient daytime conditions,
you will have to dramatically reduce the amount of ambient light striking the detector in
order to see an significant reduction in the amount of noise produced at the detector
circuit. The equation also describes that under dark nighttime conditions, the stray light
has to dramatically increase in order to produce a sizable elevation in noiseIf the system
must work during both day and night, it will have to contend with the worst daytime noise
conditions. Conversely, some light receivers could take advantage of the low stray light
conditions found at night and produce a communications system with a much longer range
than would be otherwise possible if it were used during daylight.
As mentioned above, inserting an
optical filter between the lens and the light detector can reduce the effects of ambient
light. But, as shown by the noise equation, the amount of light hitting the detector needs
to be dramatically reduced to produce a sizable reduction in the induced noise. Since most
sunlight contains a sizable amount of infrared light, such filters do not reduce the noise
level very much. However, very narrow band filters that can be selected to match the
wavelength of a laser diode light source, are effective in reducing ambient light and
OTHER RECEIVER CIRCUITS
The circuits described above were designed for a voice audio
communications system that received narrow 1uS light pulses. An experimenter may wish to
use other modulation frequencies. In addition, untuned broad band receiver circuits are
handy when monitoring modulated light signals where the frequency is not known. I have
included some additional circuits below that you may find helpful.
A very simple and inexpensive
broad band light receiver circuit is shown in PDF
Figure 6n. The circuit uses a CD4069UB C-MOS logic integrated circuit.
Make sure to use the unbuffered UB version of this popular device. The first section of
the circuit performs the current to voltage conversion. The other section provides voltage
gain. The overall conversion is about 2 volts per microwatt. With the values shown, the
circuit will work with light modulation frequencies between 1KHz and 200KHz.
|A similar circuit is shown in PDF Figure 6o. It uses a much faster 74HCU04 device
instead of the CD4069UB. The circuit should be operated from a 3v supply. For real
flexibility, I have shown how a Motorola MFOD-71 optical fiber photodiode module can be
used. The circuit's 2MHz bandwidth is great when monitoring light pulses with fast edges.
A section of inexpensive plastic optical fiber can be attached to the detector and used as
a light probe to inspect the output from various modulated light sources. Keep in mind,
that since both broad band circuits do not use an inductor in the feedback circuit, they
should only be operated in low ambient light conditions.
A very sensitive light receiver circuit, designed for
detecting the 40KHz signal used by many optical remote control devices, is shown in PDF Figure 6p. The circuit shown uses a one inch
plastic lens in conjunction with a large 10mm X 10mm photodiode. With the values
chosen, the circuit will detect light from a tpical optical remote from several hundred
feet away. If the remote control circuit also used a small lens, the separation
distance could exten several miles.