The rfRXD0420/0920 are low cost, compact single
frequency short-range radio receivers requiring only a
minimum number of external components for a
complete receiver system. The rfRXD0420 covers the
receive frequency range of 300 MHz to 450 MHz and
the rfRXD0920 covers 800 MHz to 930 MHz. The
rfRXD0420 and rfRXD0920 share a common architecture. They can be configured for Amplitude Shift Keying
(ASK), Frequency Shift Keying (FSK), or FM modulation. The rfRXD0420/0920 are compatible with rfPIC™
and rfHCS series of RF transmitters.
• High frequency stability over temperature and
power supply variations
• Low spurious signal emission
• High large-signal handling capability with
selectable LNA gain control for improved dynamic
range
• Selectable IF bandwidth via external low cost
ceramic IF filter. The IF Frequency range is
selectable between 455 kHz to 21.4 MHz. This
facilitates the use of readily available low cost
10.7 MHz ceramic IF filters in a variety of
bandwidths.
• ASK or FSK for digital data reception
• FM modulation for analog signal reception
• FSK/FM demodulation using quadrature detector
(phase coincidence detector)
• Received Signal Strength Indication (RSSI) for
signal strength indication and ASK detection
• Wide supply voltage range
• Low active current consumption
• Very low standby current
The rfRXD0420/0920 is a single conversion superheterodyne architecture. A block diagram is illustrated in
Figure 1-1. The rfRXD0420/0920 consists of:
• Low-noise amplifier (LNA) - Gain selectable
• Mixer for down-conversion of the RF signal to the
Intermediate Frequency (IF) followed by an IF
preamplifier
• Fully integrated Phase-Locked Loop (PLL)
frequency synthesizer for generation of the Local
Oscillator (LO) signal. The frequency synthesizer
consists of:
- Crystal oscillator
- Phase-frequency detector and charge pump
- High-frequency Voltage Controlled Oscillator
(VCO)
- Fixed feedback divider
- rfRXD0420 = divide by 16
- rfRXD0920 = divide by 32
• IF limiting amplifier to amplify and limit the IF
signal and for Received Signal Strength Indication
(RSSI) generation
• Demodulator (DEMOD) section consists of a
phase detector (MIXER2) and amplifier creating a
quadrature detector (also known as a phase
coincidence detector) to demodulate the IF signal
in FSK and FM modulation applications
• Operational amplifier (OPA) that can be configured as a comparator for ASK or FSK data
decision or as a filter for FM modulation.
• Bias circuitry for bandgap biasing and circuit
shutdown
DS70090A-page 2Preliminary 2003 Microchip Technology Inc.
RSSI21OAnalogReceived signal strength indicator output
OUT+23OAnalogDemodulator output (positive)
DEM
OUT-24OAnalogDemodulator output (negative)
DEM
XTAL26IAnalogCrystal oscillator input
ENRX28ICMOSReceiver enable input
LF29IAnalogExternal loop filter connection. Common node of
charge pump output and VCO tuning input.
IN31IAnalogLNA input
LNA
V
DD8, 14, 17, 27, 32PPositive supply
SS1, 5, 10, 25, 30PGround reference
V
Legend: I = Input, O = Output, I/O = Input/Output, P = Power, CMOS = CMOS compatible input or output
DS70090A-page 4Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
A
2.0CIRCUIT DESCRIPTION
This section gives a circuit description of the internal
circuitry of the rfRXD0420/0920 receiver. External
connections and components are given in the
APPLICATION CIRCUITS section.
2.1Bias Circuitry
Bias circuitry provides bandgap biasing and circuit
shutdown capabilities. The ENRX (Pin 28) modes are
summarized in Table 2-1. The ENRX pin is a CMOS
compatible input and is internally pulled down to Vss.
TABLE 2-1: BIAS CIRCUITRY CONTROL
(1)
ENRX
0Standby mode
1Receiver enabled
Note 1: ENRX has internal pull-down to Vss
2.2Frequency Synthesizer
The Phase-locked Loop (PLL) frequency synthesizer
generates the Local Oscillator (LO) signal. It consists
of:
• Crystal oscillator
• Phase-frequency detector and charge pump
• Voltage Controlled Oscillator (VCO)
• Fixed feedback divider:
- rfRXD0420 = divide by 16
- rfRXD0920 = divide by 32
Description
The PLL consists of a phase-frequency detector,
charge pump, voltage-controlled oscillator (VCO), and
fixed divide-by-16 (rfRXD0420) or divide-by-32
(rfRXD0920) divider. The rfRXD0420/0920 employs a
charge pump PLL that offers many advantages over
the classical voltage phase detector PLL: infinite pull-in
range and zero steady state phase error. The charge
pump PLL allows the use of passive loop filters that are
lower cost and minimize noise. Charge pump PLLs
have reduced flicker noise thus limiting phase noise.
An external loop filter is connected to pin LF (Pin 29).
The loop filter controls the dynamic behavior of the
PLL, primarily lock time and spur levels. The application determines the loop filter requirements.
The VCO gain for the rfRXD0420/0920 receivers are
listed in Table 2-2.
TABLE 2-2: PLL PARAMETERS
Device
K
VCO
(1)
rfRXD0420250 MHz/V at
433 MHz
rfRXD0920300 MHz/V at
868 MHz
Note 1: Typical value
The LF pin is illustrated in Figure 2-2.
(1)
ICP
Divider
60 µA16
60 µA32
FIGURE 2-2:BLOCK DIAGRAM OF LOOP
FILTER PIN
2.2.1CRYSTAL OSCILLATOR
The internal crystal oscillator is a Colpitts type oscillator. It provides the reference frequency to the PLL. A
crystal is normally connected to the XTAL (Pin 26) and
ground. The internal capacitance of the crystal oscillator is 15 pF. Alternatively, a signal can be injected into
the XTAL pin from a signal source. The signal should
be AC coupled via a series capacitor at a level of
approximately 600 mV
.
pp
The XTAL pin is illustrated in Figure 2-1.
FIGURE 2-1:BLOCK DIAGRAM OF
XTAL PIN
VDD
VDDVDD
XTAL
26
VSS
50 kΩ
30 pF
30 pF
VSSVSS
40 µ
VDD
LF
29
VSS
200 Ω
400 Ω
4 pF
VSS
VSS
2.3Low Noise Amplifier
The Low-Noise Amplifier (LNA) is a high-gain amplifier
whose primary purpose is to lower the overall noise
figure of the entire receiver thus enhancing the receiver
sensitivity. The LNA is an open-collector cascode
design. The benefits of a cascode design are:
• high gain with low noise
• high-frequency
• wide bandwidth
• low effective input capacitance with stable input
impedance
• high output resistance
• high reverse isolation that provides improved
stability and reduces LO leakage
Approximate LNA noise figures are listed in Table 2-3.
TABLE 2-3: LNA NOISE FIGURES
Device
Noise Figure
rfRXD0420TBD
rfRXD0920TBD
Note 1: Approximate value
LNA
IN (Pin 31) has an input impedance of approxi-
mately 26 Ω || 2 pF single-ended.
OUT (Pin 3) has an open-collector output and is
LNA
pulled up to V
DD via a tuned circuit.
Important: To ensure LNA stability the V
must be connected to a low impedance ground.
The LNA pins are illustrated in Figure 2-3.
(1)
SS pin (Pin 1)
FIGURE 2-3:BLOCK DIAGRAM OF LNA
PINS
LNA
VSS
V
VSS
OUT
3
DD
VSS
1
LNA
31
1.6V
0.8V
VDD
5 kΩ
IN
VSS
The gain of the LNA can be selected between High and
Low Gain modes by the LNA
GAIN pin (Pin 2). LNAGAIN
is a CMOS input with hysteresis. Table 2-4 summarizes
the voltage levels and modes for LNA gain.
In the High Gain mode the LNA operates normally. In
Low Gain mode the gain of the LNA is reduced approximately 25 dB, reduces total supply current, and
increases maximum input signal levels (see Electrical
Characteristics section for values).
TABLE 2-4: LNA GAIN CONTROL
LNAGAINDescription
< 0.8 VHigh Gain mode
> 1.4 VLow Gain mode
The 1IF+ (Pin 6) and 1IF- (Pin 7) are bias connections
to the MIXER1 balanced collectors. Both pins are
open-collector outputs and are individually pulled up to
DD by a load resistor. The MIXER1 bias pins are illus-
V
trated in Figure 2-5.
1IF
OUT (Pin 9) has an approximately 330 Ω single-
ended output impedance. The 330 Ω impedance
provides a direct match to low cost ceramic IF filters.
The 1IF
OUT pins is illustrated in Figure 2-6.
FIGURE 2-4:BLOCK DIAGRAM OF MIXER1
PIN
1IF
4
VDD
IN
VSS
13 Ω
13 Ω
500 µA
VSS
FIGURE 2-5:BLOCK DIAGRAM OF MIXER1
BIAS PINS
VDDVDD
VSS
20 pF
500 µA
1IF-
7
VSS
1IF+
6
20 pF
VSS
500 µA
VSS
FIGURE 2-6:BLOCK DIAGRAM OF IF
PREAMP PIN
VDDVDD
6.8 kΩ
130 Ω
230 µA
VSS
1IF
9
VDD
OUT
VSS
2.5IF Limiting Amplifier with RSSI
2.4MIXER1 and IF Preamp
MIXER1 performs down-conversion of the RF signal to
the Intermediate Frequency (IF) and is followed by an
The IF Limiting Amplifier amplifies and limits the IF
signal at the 2IF
IN pin (Pin 11). It also generates the
Received Signal Strength Indicator (RSSI) signal
(Pin 21).
IF preamplifier.
IN (Pin 4) has an approximately 33 Ω single-ended
1IF
input impedance. The 1IF
IN pin is illustrated in Figure 2-
4.
2.5.1IF LIMITING AMPLIFIER
Magnitude control circuitry is used in the last stage of
the receiver to keep the signal constant for demodulation. It can consist of a limiting or Automatic Gain
Control (AGC) amplifier. A limiting amplifier is
DS70090A-page 6Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
employed in this design because it can handle a larger
dynamic range while consuming less power with simple
circuitry than AGC circuitry.
The internal resistance of the 2IF
IN pin is approximately
2.2 kΩ. In order to terminate ceramic IF filters whose
output impedance is 330 Ω, a 390 Ω resistor can be
paralleled to the 2IF
IN and FBC2 pins.
FBC1 (Pin 12) and FBC2 (Pin 13) are connected to
external feedback capacitors.
The IF Limiting Amplifier pins are illustrated in
Figures 2-7 and 2-8.
FIGURE 2-7:BLOCK DIAGRAM OF IF
LIMITING AMPLIFIER INPUT
PINS
2IF
11
FBC2
13
VDD
IN
VSS
VDD
VSS
2.2 kΩ
2.2 kΩ
200 µA
Vss
VDD
FBC1
12
VSS
FIGURE 2-8:BLOCK DIAGRAM OF IF
LIMITING AMPLIFIER OUTPUT
PIN
VDD
VDD
OUT
2IF
15
VSS
40 µA
VSS
2.5.2RECEIVED SIGNAL STRENGTH
INDICATOR (RSSI)
The RSSI signal is proportional to the log of the signal
at 2IF
IN. The 2IFIN input RSSI range is approximately
40 µV to 160 mV. The slope of the RSSI output is
approximately 26 mV/dB of RF signal.
The RSSI output has an internal 36 kΩ resister to Vss
fed by a current source. This resistor converts the
RSSI current to voltage.
For Amplitude Shift Keying (ASK) demodulation, RSSI
is compared to a reference voltage (static or dynamic).
Post detector filtering is easily implemented by
connecting a capacitor to ground from the RSSI pin
effectively creating an RC filter with the internal 36 kΩ
resistor.
For FSK and FM demodulation, the RSSI represents
the received signal strength of the incoming RF signal.
The RSSI pin is illustrated in Figure 2-9.
FIGURE 2-9:BLOCK DIAGRAM OF RSSI
PIN
VDD
RSSI
21
50 Ω
VSS
I (Pi)
36 kΩ
VSS
2.6Demodulator
The demodulator (DEMOD) section consists of a phase
detector (MIXER2) and amplifier creating a quadrature
detector (also known as a phase coincidence detector)
to demodulate the IF signal in FSK and FM modulation
applications. The quadrature detector provides all the
IF functions required for FSK and FM demodulation
with only a few external parts.
The in-phase signal comes directly from the output of
the IF limiting amplifier to MIXER2. The quadrature
signal is created by an external tuned circuit from the
output of the IF limiting amplifier (2IF
coupled to the MIXER2 DEM
impedance of the DEM
IN (Pin 16) input. The input
IN pin is approximately 47 kΩ.
The external tuned circuit can be constructed from simple inductor-capacitor (LC) components but will require
one of the elements to be tunable. A no-tune solution
can be constructed with a ceramic discriminator.
The output voltage of the DEMOD amplifier (DEMout+
and DEMout-, Pins 23 and 24) depends on the peak
deviation of the FSK or FM signal and the Q of the
external tuned circuit. DEMout+ and DEMout- are high
impedance outputs with only a 20 µA current capability.
The Demodulator pins are illustrated in Figures 2-10
and 2-11.
The internal operational amplifier (OPA) can be
configured as a comparator for ASK or FSK or as a filter
for FM modulation applications.
The Op Amp pins are illustrated in Figures 2-12 and
2-13.
FIGURE 2-12: BLOCK DIAGRAM OF OP AMP
INPUT PINS
VDD
VDDVDD
OPA-
19
50 Ω50 Ω
VSSVSS
20 µA
OPA+
20
FIGURE 2-13: BLOCK DIAGRAM OF OP AMP
OUTPUT PIN
VDD
OPA
18
VSS
VDD
50 Ω
VSS
DS70090A-page 8Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
)
3.0APPLICATION CIRCUITS
This section provides general information on application circuits for the rfRXD0420/0920 receiver. The
following connections and external components
provide starting points for designs and list the minimum
circuitry recommended for general purpose
applications.
Performance of the radio system (transmitter and
receiver) is affected by component selection and the
environment in which it operates. Each system design
has its own unique requirements. Specifications for a
particular design requires careful analysis of the application and compromises for a practical implementation.
3.1General
This subsection lists connections and components that
are common between applications. The following
subsections give specific circuit connections and
components for ASK, FSK and FM applications.
3.1.1BYPASS CAPACITORS
Bypass capacitors should be placed as physically close
as possible to V
respectively. Additional bypassing and board level lowpass filtering of the power supply may be required
depending on the application.
3.1.2FREQUENCY PLANNING
The rfRXD0420/0920 receivers are single-conversion
superheterodyne architecture with a single IF
frequency. The receive frequency is set by the crystal
frequency (f
a majority of applications an external crystal is
connected to XTAL (Pin 26). Figure 3-1 illustrates an
example circuit with an optional trim capacitor.
FIGURE 3-1:XTAL EXAMPLE CIRCUIT
DD pins 8, 14, 17, 27 and 32
) and intermediate frequency (fif). For
XTAL
WITH OPTIONAL TRIM
CAPACITOR
XTAL
26
C TRIM
(OPTIONAL
X1
effect the trim capacitor has on the receive frequency
for the rfRXD0420 at 433.92 MHz. Keep in mind that
this graph represents one example circuit and the
actual results depends on the crystal and PCB layout.
FIGURE 3-2:RECEIVE FREQUENCY VS.
TRIM CAPACITANCE
434.10
434.05
434.00
433.95
433.90
433.85
433.80
Receive Frequency (MHz)
433.75
82 pF
0 ohms
68 pF
56 pF
47 pF
Trim Capacitor (pF)
39 pF
33 pF
27 pF
22 pF
18 pF
15 pF
12 pF
10 pF
5 pF
Note that a 0 Ω resistor, in the lower left of the graph,
represents an infinite capacitance. This will be the
lowest frequency obtainable for the crystal and PCB
combination.
Calculation of the crystal frequency requires knowledge of the receive frequency (f
frequency (f
). Figure 3-3 is a worksheet to assist the
if
) and intermediate
rf
designer in calculating the crystal frequency. Table 3-1
lists crystal frequencies for popular receive frequencies. Table 3-2 lists crystal parameters required for
ordering crystals. For background information on
crystal selection see Application Note AN826, Crystal
Oscillator Basics and Crystal Selection for rfPIC
PICmicro
®
Devices.
TM
and
TABLE 3-1: CRYSTAL FREQUENCIES FOR
POPULAR RECEIVE
FREQUENCIES
Receive
Frequency
rfRXD0420
315 MHz20.35625 MHz
433.92 MHz26.45125 MHz
rfRXD0920
868.3 MHz26.8 MHz
915 MHz28.259375 MHz
(1) Low-side injection (2) High-side injection
Crystal
Frequency
(2)
(1)
(1)
(1)
TABLE 3-2: CRYSTAL PARAMETERS
ParameterValue
The crystal load capacitance should be specified to
include the internal load capacitance of the XTAL pin of
15 pF plus PCB stray capacitance (approximately 2 to
3 pF). A trim capacitor can be used to trim the crystal
on frequency within the limitations of the crystal’s trim
sensitivity and pullability. Figure 3-2 illustrates the
=___________ + ( 2 x ___________ )= ______________
=___________ - ( 2 x ___________ )= ______________
=_________ x
) for the Injection mode chosen:
16 if rfRXD0420
32 if rfRXD0920
) that corresponds to the LO frequency
lo-LOW
(circle one)
= _____________
) and circle
XTAL
DS70090A-page 10Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
3.1.3PLL LOOP FILTER
An external PLL loop filter is connected to pin LF
(Pin 29). The loop filter controls the dynamic behavior
of the PLL, primarily lock time and spur levels. Generally, the PLL lock time is a small fraction of the overall
receiver start-up time (see Electrical Characteristics
Section). The crystal oscillator is the largest contributor
to start-up time. Thus, for the majority of applications,
design loop filter values for a wide loop bandwidth to
suppress noise. Figure 3-4 illustrates an example filter
circuit for a wide frequency range suitable for a majority
of applications.
FIGURE 3-4:PLL LOOP FILTER EXAMPLE
CIRCUIT
LF
29
C2
C1
1000 pFOPTIONAL
R1
10 kΩ
3.1.4PRESELECTOR
Receiver performance is heavily influenced by the
preselector (also known as the front-end filter). The
purpose of the preselector is to filter unwanted signals
and noise from entering the receiver.
The most important unwanted signal is the image
frequency (f
image frequency calculated in Figure 3-3 as this will be
the frequency that needs to be filtered out by the
preselector.
The preselector can be designed using a simple LC
filter or a Surface Acoustic Wave (SAW) filter. A simple
LC filter provides a low cost solution but will have the
least effect filtering the image frequency. A SAW filter
can effectively filter the image frequency with a
minimum of 40 dB attenuation.
). Pay particular attention to the
rf-image
The SAW filter has the added advantage of filtering
wide-band noise and improving the signal-to-noise
ratio (SNR) of the receiver.
SAW filters require impedance matching. Refer to the
manufacturers' data sheet and application notes for
SAW filter pinouts, specified impedances and recommended matching circuits. Figure 3-5 shows a SAW
filter example circuit.
A secondary purpose of the preselector is to provide
impedance matching between the antenna and LNA
(Pin 31).
3.1.5ANTENNA
Receiver performance and device packaging influence
antenna selection. There are many third-party antennas to choose from. Third-party antennas typically
have an impedance of 50 Ω. The preselector components should be chosen to match the impedance of the
antenna to the LNA
IN (Pin 31) impedance of
26 Ω || 2 pF.
The designer can chose to use a simple wire antenna.
The length of the wire should be one-quarter the wavelength (λ) of the receive frequency. For example, the
wavelength of 433.92 MHz is:
λ = c / f
λ = 3 x 10
where c = 3 x 108 m/s
rf
8
m/s / 433.92 x 106 Hz
λ = 0.69 m
therefore
0.25λ = 17.3 cm or 6.8 inches
Finally, the wire antenna should be impedance
matched to the preselector. The typical impedance of a
one-quarter wavelength wire antenna is 36 Ω.
3.1.6LNA GAIN
For a majority of applications, LNAGAIN can be tied to
Vss (ground) enabling High Gain mode. If the application requires short range communications, LNA
can be tied to VDD (pulled up) enabling Low Gain mode.
More Information on LNA
GAIN operation can be found
in the Circuit Description section.
GAIN
IN
FIGURE 3-5:SAW FILTER EXAMPLE CIRCUIT
L1L2
C1C2
2
Input
1
Input Gnd
Note:Refer to SAW filter manufacturer’s data sheet for pin outs
The LNAOUT (Pin 3) has an open-collector output. It is
pulled up to V
IN (Pin 4) via a series decoupling capacitor. The
to 1IF
IN input impedance is approximately 33 Ω || 1.5 pF.
1IF
Important: To ensure LNA stability the V
DD via a tuned circuit. It is also connected
SS pin (Pin 1)
must be connected to a low impedance ground.
As shown in Figure 3-6, components C1 and L1 make
up the tuned circuit and provide collector current via
pull-up. Together with decoupling capacitor C2, they
provided impedance matching between the LNA and
MIXER1. To a lesser extent, C1, L1, and C2 provide
band-pass filtering at the receive frequency (f
).
rf
Component values depend on the selected receive
frequency. The challenge is to design the circuit with
the fewest components setting Q as high as possible
as limited by component tolerances. For a majority of
applications it is best to design a wide bandwidth tuned
circuit to account for manufacturing and component
tolerances. The best approach is to design the tuned
circuit using a filter simulation program. Table 3-3 lists
example component values for popular receive
frequencies.
FIGURE 3-6:LNA OUTPUT TO MIXER1
EXAMPLE CIRCUIT.
VDD
C Bypass
C1C2L1
34
OUT
LNA
IN
1IF
TABLE 3-3: LNA TUNED CIRCUIT EXAMPLE
COMPONENT VALUES
f
rf
315 MHz7.0 pF22 nH6.0 pF
433.92 MHz3.0 pF15 nH6.0 pF
868.3 MHz2.0 pF7.6 nH3.0 pF
915 MHz2.0 pF6.8 nH3.0 pF
These values are for design guidance only.
C1L1C2
3.1.8MIXER1 BIAS
The 1IF+ (Pin 6) and 1IF- (Pin 7) are bias connections
to the MIXER1 balanced collectors. Both pins are
open-collector outputs and are individually pulled up to
DD by a load resistor. Figure 3-7 shows a MIXER1
V
bias example circuit.
FIGURE 3-7:MIXER1 BIAS EXAMPLE
CIRCUIT
VDDVDD
R1
470 Ω
1IF+
R2
470 Ω
76
1IF-
3.1.9INTERMEDIATE FREQUENCY (IF)
FILTER
The IF filter defines the overall adjacent signal selectivity of the receiver. For a majority of applications, lowcost 10.7 MHz ceramic IF filters are used. These are
available in a variety of bandwidths and packages.
IF filter bandwidth selection is a function of:
• modulation (ASK, FSK or FM)
• signal bandwidth
• frequency and temperature tolerances of the
transmitter and receiver components
The typical input and output impedance of ceramic
filters is 330 Ω. 1IF
OUT (Pin 9) has an approximately
330 Ω single-ended output impedance and provides a
direct match to the ceramic IF filter. The internal resistance of the 2IF
IN (Pin 11) is approximately 2.2 kΩ. In
order to terminate ceramic IF filters a 390 Ω resistor
can be paralleled to the 2IF
IN and FBC2 (Pin 13).
Figure 3-8 shows an example circuit schematic using a
10.7 MHz ceramic IF filter.
3.1.10 IF LIMITING AMPLIFIER EXTERNAL
FEEDBACK CAPACITORS
FBC1 (Pin 12) and FBC2 (Pin 13) are connected to
external feedback capacitors. Figure 3-8 shows
component values and connections for these
capacitors.
DS70090A-page 12Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
+
-
FIGURE 3-8:IF FILTER, LIMITING AMPLIFIER AND DEMODULATOR BLOCK DIAGRAM
DS70090A-page 14Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
3.2Amplitude Shift Keying (ASK)
Figure 3-9 illustrates an example ASK applications circuit.
The IF Limiting Amplifier with RSSI is used as an ASK
detector. The RSSI signal is post detector filtered and
then compared to a reference voltage to determine if
the incoming RF signal is a logical one or zero. The
reference voltage can be configured as a dynamic
voltage level determined by the incoming RF signal
strength or by a predetermined fixed level.
3.2.1RSSI POST DETECTOR FILTERING
The RSSI signal is low-passed filtered to remove high
frequency and pulse noise to aid the decision making
process of the comparator and increase the sensitivity
of the receiver. The RSSI signal low-pass filter is a RC
filter created by the RSSI output impedance of 36 kΩ
and capacitor C1. Setting the time constant (RC = τ) of
the RC filter depends on the signal period and when the
signal decision will be made.
3.2.1.1Signal Period
Optimum sensitivity of the receiver with reasonable
pulse distortion occurs when the RC filter time constant
is between 1 and 2 times the signal period. If the time
constant of the RC filter is set too short, there is little
noise filtering benefit. However, if the time constant of
the RC filter is set too long, the data pulses will become
elongated causing inter-symbol interference.
3.2.1.2Signal Decision
If the bit decision occurs in the center of the signal
period (such as K
times the RC filter time constant should be set at less
than or equal to half the signal period. Figure 3-10 illustrates this method. The top trace represents the
received on-off keying (OOK) signal. The bottom trace
shows the RSSI signal after the RC low-pass filter.
FIGURE 3-10: CENTER SIGNAL PERIOD
OOK Signal
RSSI Signal
EELOQ decoders), then one or two
DECISION RSSI LOW-PASS
FILTERED
Signal Decision
Signal Period
1τ to 2τ
If the bit decision occurs near the end of the signal
period, then the time constant should be set at less
than or equal to the signal period. Figure 3-11
illustrates this method.
Once the signal decision time and time period of the
signal period are known, then capacitor C1 can be
selected. Once C1 is selected, the designer should
observe the RSSI signal with an oscilloscope and
perform operational and/or bit error rate testing to
confirm receiver performance.
FIGURE 3-11: NEAR END OF THE SIGNAL
PERIOD DECISION RSSI LOWPASS FILTERED
Signal Decision
OOK Signal
Signal Period
RSSI Signal
1τ to 2τ
3.2.2COMPARATOR
The internal operational amplifier is configured as a
comparator. The RSSI signal is applied to OPA+ (Pin
20) and compared with a reference voltage on OPA(Pin 19) to determine the logic level of the received
signal. The reference voltage can be dynamic or static.
The choice of dynamic versus static reference voltage
depends in part on the ratio of logical ones versus
zeros of the data (this can also be thought of as the AC
content of the data). Provided the ratio has an even
number of logical ones versus zeros, a dynamic reference voltage can be generated with a simple low-pass
filter. The advantage of the dynamic reference voltage
is the increased receiver sensitivity compared to a fixed
reference voltage. However, the comparator will output
random data. The decoder (for example, a programmed PICmicro MCU or K
distinguish between random noise and valid data.
The choice of a static reference voltage depends in part
on the DC content of the data. That is, the data has an
uneven number of logical ones versus zeros. The
disadvantage of the static reference voltage is
decreased receiver sensitivity compared to a dynamic
reference voltage. In this case, the comparator will
output data without random noise.
A dynamic reference voltage can be derived by averaging the received signal with a low-pass filter. The example ASK application circuit shown in Figure 3-9, the
low-pass filter is formed by R1 and C2. The output of
the low-pass filter is then fed to OPA-.
The setting of the R1-C2 time constant depends on the
ratio of logical ones versus zeros and a trade off in
stability versus receiver reaction time. If the received
signal has an even number of logical ones versus
zeros, the time constant can be set relatively short.
Thus the reference voltage can react quickly to
changes in the received signal amplitude and differences in transmitters. However, it may not be as stable
and can fluctuate with the ratio of logical ones and
zeros. If the time constant is set long, the reference
voltage will be more stable. However, the receiver
cannot react as quickly upon the reception of a
received signal.
Selection of component values for R1 and C2 is an
iterative process. First start with a time constant
between 10 to 100 times the signal rate. Second, view
the reference voltage against the RSSI signal to
determine if the values are suitable. Figure 3-12 is an
oscilloscope screen capture of an incoming RF square
wave modulated signal (ASK on-off keying). The top
trace is the data output of OPA (Pin 18). The two
bottom traces are the RSSI signal (Pin 21, bottom
square wave) and generated reference voltage (Pin 19,
bottom trace centered in the RSSI square wave). The
goal is to select values for R1 and C2 such that the
reference voltage is in the middle of the RSSI signal.
This reference voltage level provides the optimum data
comparison of the incoming data signal.
3.2.2.2STATIC REFERENCE VOLTAGE
A static reference voltage can be derived by a voltage
divider network.
FIGURE 3-12:RSSI AND REFERENCE VOLTAGE COMPARISON
OPA
(Pin 18)
OPA-
(Pin 19)
RSSI
(Pin 21)
DS70090A-page 16Preliminary 2003 Microchip Technology Inc.
Figure 3-13 illustrates an example FSK application
circuit.
3.3.1IF FILTER CONSIDERATIONS
As mentioned in the Section 3.1 above, IF filter bandwidth selection is a function of:
• modulation (ASK, FSK or FM)
• signal bandwidth
• frequency and temperature tolerances of the
transmitter and receiver components
The occupied bandwidth of binary FSK signals is 2
times the peak frequency deviation plus 2 times the
signal bandwidth. For example, if the data rate is 2400
bits per second Manchester encoded, the signal bandwidth is 4800 baud or 1200 Hz, and if the peak
frequency deviation is 24 kHz, the minimum bandwidth
of the IF filter is:
IF BW
IF BW
Add to this value the frequency and temperature
tolerances of the transmitter and receiver components.
FSK signals are more sensitive to group delay variations of the IF filter. Therefore, a filter with a low group
delay variation should be used. As an alternative, a
filter with wider than required bandwidth can be used
because the group delay variation in the center of the
bandpass will be relatively constant.
3.3.2FSK DETECTOR
The demodulator (DEMOD) section consists of a phase
detector (MIXER2) and amplifier creating a quadrature
detector (also known as a phase coincidence detector)
to demodulate the IF signal in FSK and FM modulation
applications. The in-phase signal comes directly from
the output of the IF limiting amplifier to MIXER2. The
quadrature signal is created by an external tuned circuit
from the output of the IF limiting amplifier (2IF
15) AC-coupled to the MIXER2 DEM
3.3.2.1LC Discriminator
The external tuned circuit can be constructed from
simple inductor-capacitor (LC) components. This type
circuit produces and excellent output. However, one of
the elements (L or C) must be tunable. Figure 3-14
illustrates an example LC discriminator circuit using a
tunable capacitor. A similar circuit with a tunable inductor is also possible. Resistor R1 = 4.7 kΩ reduces the
Q of the circuit so that frequency deviations of up to 75
kHz can be demodulated.
= (2 x 2400) + (2 x 24000)
min
= 52800 Hz
min
OUT, Pin
IN (Pin 16) input.
FIGURE 3-14: LC DISCRIMINATOR
EXAMPLE CIRCUIT
R1
4.7 kΩ
C3
0-56 pF
C1
1.0 pF
OUT
2IF
1615
C2
680 pF
IN
DEM
L1
3.3 µH
3.3.2.2Ceramic Discriminator
A no-tune solution can be constructed with a ceramic
discriminator. Figure 3-15 illustrates an example
ceramic discriminator circuit.
The ceramic discriminator acts as a parallel tuned
circuit at the IF frequency (for example, 10.7 MHz). The
parallel capacitor C3 tunes the ceramic resonator. The
high Q of this circuit enables higher output of the detector for small frequency deviations. However, smaller
frequency deviations require better frequency
tolerances at the transmitter and receiver.
In order to detect wider deviation or off-frequency
signals, the detector bandwidth has to be increased.
This can be accomplished by reducing the Q of the
tuned circuit. One method is to parallel a resistor
across the ceramic discriminator. A second is to
increase the value of the coupling capacitor C1
increasing the load on the detector. The result of
reducing the Q of the discriminator will be that the
detector output will be smaller.
FIGURE 3-15: CERAMIC DISCRIMINATOR
EXAMPLE CIRCUIT
C2
680 pF
IN
DEM
F1
C3
10-12 pF
CERAMIC DISCRIMINATOR
C1
1.0 pF
1615
OUT
2IF
DS70090A-page 18Preliminary 2003 Microchip Technology Inc.
3.3.3POST DETECTOR FILTERING
Care should be taken in selecting the values of capacitors C1 and C2 (Figure 3-13) so that the output of the
detector is not distorted and receiver sensitivity
improved. These values are chosen depending on the
data signal rate.
Generally, if the data signal rate is fast then the filter
time constant can be set short. Conversely, if the signal
rate is slow, the filter time constant can be set long. The
designer should observe the output of the detector with
an oscilloscope and perform operational and/or bit
error rate testing to confirm receiver performance.
3.3.4COMPARATOR
The output of the DEMOD amplifier (DEMOUT+ and
OUT-, Pins 23 and 24) depends on the peak
DEM
deviation of the FSK or FM signal and the Q of the
external tuned circuit. DEMout+ and DEMout- are high
impedance outputs with only a 20 µA current capability.
The capacitance on these pins limit the maximum data
signal rate. The nominal output voltage of these pins is
DS70090A-page 20Preliminary 2003 Microchip Technology Inc.
3.4Frequency Modulation (FM)
Figure 3-16 illustrates an example FM application
circuit.
3.4.1FSK DETECTOR
FM demodulation is performed in the same manner as
described in the FSK section above.
3.4.2OPERATIONAL AMPLIFIER
The internal operational amplifier is configured as an
active low-pass filter.
FM audio is typically de-emphasized. It is recommended that de-emphasis circuitry be connected at the
output of the operational amplifier rather than the
output of the detector.
Supply voltage...................................................................................................................................................0 to +7.0V
Input voltage...........................................................................................................................................-0.3 to V
Storage temperature .................................................................................................................................... -40 to +125C
† NOTICE: Stresses above those listed under “Absolute Maximum Ratings” may cause permanent damage to the
device. This is a stress rating only and functional operation of the device at those or any other conditions above those
indicated in the operation listings of this specification is not implied. Exposure to maximum rating conditions for
extended periods may affect device reliability.
CC+0.3V
DS70090A-page 22Preliminary 2003 Microchip Technology Inc.
4.1DC Characteristics: rfRXD0420
(Industrial)
rfRXD0420/0920
DC CHARACTERISTICS
Param
No.
SymCharacteristicMinTyp
V
CCSupply Voltage2.5—5.5Vf
STBYStandby Current100nAENRX = 0
I
CCSupply Current5.06.58.0mALNAGAIN = 1
I
OPAOp Amp input voltage offset-20—20mV
V
OPAOp Amp input current offset-50—50nA
I
BIASOp Amp input bias current-100100nA
I
RSSIRSSI voltage0.51.01.5VLNAGAIN = 1
V
Standard Operating Conditions (unless otherwise stated)
Operating Temperature -40°C ≤ T
†
MaxUnitsConditions
2.7—5.5Vf
6.58.210.0mALNA
1.251.92.45VLNA
A ≤ +85°C
< 400 MHz
rf
> 400 MHz
rf
GAIN = 0
GAIN = 0
*These parameters are characterized but not tested.
†
Data in “Typ” column is at 3V, 23°C unless otherwise stated. These parameters are for design guidance only and
are not tested.
4.2AC Characteristics: rfRXD0420
(Industrial)
AC CHARACTERISTICS
Standard Operating Conditions (unless otherwise stated)
*These parameters are characterized but not tested.
†
Data in “Typ” column is at 3V, 23°C, frf = 433.6 MHz, IF = 10.7 MHz unless otherwise stated. These parameters
are for design guidance only and are not tested.
Note 1: Dependant on ASK detector time constant.
2: IF bandwidth = 40 kHz, ∆f = +/- 15 kHz, BER <= 3 x 10
3: IF bandwidth = 150 kHz, ∆f = +/- 50 kHz, BER <= 3 x 10
4: IF bandwidth = 40 kHz, BER <= 3 x 10
5: IF bandwidth = 150 kHz, BER <= 3 x 10
*These parameters are characterized but not tested.
†
Data in “Typ” column is at 3V, 23°C, frf = 433.6 MHz, IF = 10.7 MHz unless otherwise stated. These parameters
are for design guidance only and are not tested.
Note 1: Dependant on ASK detector time constant.
2: IF bandwidth = 40 kHz, ∆f = +/- 15 kHz, BER <= 3 x 10
3: IF bandwidth = 150 kHz, ∆f = +/- 50 kHz, BER <= 3 x 10
4: IF bandwidth = 40 kHz, BER <= 3 x 10
5: IF bandwidth = 150 kHz, BER <= 3 x 10
-3
-3
-3
-3
DS70090A-page 24Preliminary 2003 Microchip Technology Inc.
5.0 PACKAGING INFORMATION
5.1Package Marking Information
rfRXD0420/0920
32-Lead LQFP
XXXXXXXXXXXX
XXXXXXXXXXXX
XXXXXXXXXXXX
YYWWNNN
Legend: XX...X Customer specific information*
YYear code (last digit of calendar year)
YYYear code (last 2 digits of calendar year)
WWWeek code (week of January 1 is week ‘01’)
NNNAlphanumeric traceability code
Example
rfRXD0420
02123ABC
Note:In the event the full Microchip part number cannot be marked on one line, it will
be carried over to the next line thus limiting the number of available characters
for customer specific information.
*Standard PICmicro device marking consists of Microchip part number, year code, week code, and
traceability code. For PICmicro device marking beyond this, certain price adders apply. Please check
with your Microchip Sales Office. For QTP devices, any special marking adders are included in QTP
price.
The following section gives the technical details of the package.
32-Lead Plastic Low Profile Quad Flat Package (LQ) 7 x 7 x 1.4 mm Body
Not available at this time.
DS70090A-page 26Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
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DS70090A
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DS70090A-page 28Preliminary 2003 Microchip Technology Inc.
rfRXD0420/0920
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DS70090A-page30Preliminary 2003 Microchip Technology Inc.
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•There are dishonest and possibly illegal methods used to breach the code protection feature. All of these methods, to our
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