
General RF Electronics Answers to RF Cafe Quiz #2


Return to RF Cafe Quiz #2
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 particularly those who are fresh out of school or are relatively new to the work world. Come to
think of it, they would make equally excellent study material for the same persons who are going to
be interviewed for a job.
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in the monthly RF Cafe Giveaway.
Note: Many answers contain passages quoted in whole or in part from the text.
1. On a Smith chart, what does a
point in the bottom half of the chart represent?
b) A capacitive impedance
Points in the bottom half
of the Smith chart represent capacitive impedances while points in the top half represent inductive impedances.
Both cases include a resistive component, also. Points that lie along the center horizontal represent pure
resistances.
2. While we're on the subject of Smith charts, what is the impedance of the point at the far left edge
of the center horizontal line?
b) Zero ohms (short circuit) The Smith chart's bordering circle is the
locus of points whose reflection coefficients are of magnitude one. Here are a few of the major points on the
Smith chart (50 Ω system):
1. Left center : short circuit (0 ± j0 Ω). 2. Top center : pure inductive
reactance (0 + j50 Ω). 3. Right center : open circuit (0 ± j∞ Ω). 4. Bottom center : pure capacitive
reactance (0  j50 Ω). 5. Dead center : pure 50 ohms (50 ± j0 Ω).
3. A singleconversion
downconverter uses a highside local oscillator (LO) to translate the input radio frequency (RF) to an
intermediate frequency (IF). Will spectral inversion occur at IF?
a) Yes, always
Spectral inversion
occurs when high frequencies within the input signal bandwidth are translated to low frequencies in the output
bandwidth, and vice versa. Since a downconversion is being performed, the lower sideband of the mixing process is
extracted, hence the difference between the LO frequency and the RF frequency is desired. Consider the following
parameters and how spectral inversion occurs.
RF input frequency band : fc = 1250 MHz, BW = 100 MHz (1200  1300 MHz). LO frequency : 1600 MHz. IF
output frequency band : fc = 350 MHz, BW = 100 MHz (300  400 MHz).
When the lower frequency of the input
band is subtracted from the LO frequency (1600 MHz  1200 MHz = 400 MHz) a larger frequency is obtained than when
the higher frequency of the input band is subtracted from the LO frequency (1600 MHz  1300 MHz = 300 MHz). This
means that the output spectrum is the mirror image of the input spectrum.
How to avoid spectral inversion?
Always use a lowside LO (LO frequency below RF input frequency band) for mixing, or ensure that an even number of
spectral inversions are performed in the converter (i.e., two stages of conversion with highside LO's).
4. What happens to the noise floor of a spectrum analyzer when the input filter resolution bandwidth is decreased
by two decades?
b) 20 dB decrease
The input filter bandwidth determines the amount of power that will be present at the
detector circuitry. Since the detector performs a power integration function, it sums all of the incident power
across the band. Decreasing the bandwidth by a factor of 100 (two decades) allows one onehundredth of the amount
of power to reach the detector, which in term of decibels is:
10*log( 1/100) = 20 dB.
5.
What is a primary advantage of a quadrature modulator?
c) Singlesideband output
A quadrature
modulator is comprised of two mixers, each of which receives input data and local oscillator (LO) signals that are
shifted 90 degrees relative to each other. The outputs are summed together to generate the singlesideband signal.
Deviation of the phases from the ideal 90 degrees and deviations from equal amplitudes going into the mixers will
result in less than perfect undesired sideband cancellation. Which sideband gets canceled depends on the phase
relationship of the signals entering the mixers.
The two mixer outputs are: m1 (t) = cos
(ωL*t) * cos (ωI*t) = 1/2 * cos (ωL*t  ωI*t) + 1/2 *cos (ωL*t + ωI*t) m2 (t) = cos (ωL*t  pi/2) * cos (ωI*t
pi/2) = sin (ωL*t) * sin (ωI*t) = 1/2 * cos (ωL*t  ωI*t)  1/2 *cos (ωL*t + ωI*t)
Now sum
the m1 (t) and m2 (t) outputs: f (t) = 1/2 * cos (ωL*t  ωI*t) + 1/2 *cos (ωL*t + ωI*t) + 1/2 * cos (ωL*t 
ωI*t)  1/2 *cos (ωL*t + ωI*t) f (t) = cos (ωL*t  ωI*t)
Note that what remains is the lower sideband.
Upper sideband cancellation can be achieved by rearranging the 90 degree power splitters. If the data input is
digital, the data streams can be digitally shifted by 90 degrees and the first 90 degree power splitter can be
eliminated.
6. What is meant by dBi as applied to antennas?
c) Gain relative to an
isotropic radiator
An isotropic radiator (antenna) emits electromagnetic energy equally in all directions
as if it were originating from a point source. Equipotential surfaces are spheres with the isotropic radiator at
the center. If the antenna is designed to concentrate a majority of its energy in one or more directions, it is
said to be directional. Since the directional antenna radiates the same total power as it would if it were an
isotropic radiator, gain exists in the direction(s) of power concentration. That gain is measured in decibels
relative to an isotropic radiator (dBi).
7. What is the power dynamic range of an ideal 12bit
analogtodigital converter (ADC)?
c) 72.25 dB
An ideal 12bit ADC can assume 2^{12} (4,096) unique voltage levels. Since
power is proportional to the square of the voltage, the maximum power sample value is 4096^{2}
(16,777,216) times the minimum power sample value. Therefore the dynamic range is 10*log (16,777,216) = 72.25 dB.
A rule of thumb is 6 dB per bit.
8. An ideal 10 dB attenuator is added in front of a load that has
a 2.00:1 VSWR. What is the resulting VSWR of the load + attenuator?
a) 1.07:1
VSWR is related to
return loss (RL) according to VSWR = [10^(RL/20) + 1] / [10^(RL/20)  1]. It follows that increasing the return
loss will result in a lower VSWR. The RL of a 2.00:1 VSWR is 9.542 dB. Add the 10 dB attenuator for a total RL of
2*10 dB + 9.542 dB = 29.542 dB. Convert back to VSWR using the given formula for a value of 1.07:1.
Why add
twice the attenuator value to the return loss? Return loss is the total decrease in signal strength in passing
through the attenuator and being reflected back through the attenuator. Hence, the signal is decreased by twice
the attenuator value.
9. What is the thermal noise power in a 1 MHz bandwidth when the system
temperature is 15 °C (assume gain and noise figure are 0 dB)?
a) 114.0 dBm (in a 1 MHz BW)
Thermal
noise power density is governed by the equation 10*log (k*T*B*1000) dBm, where k is the Boltzmann constant. T is
the temperature in degrees Kelvin, and B is the bandwidth in Hertz. Multiplication by 1000 is to convert watts to
milliwatts. A rule of thumb for temperatures near 15 °C is to begin with a thermal noise density of 174 dBm/Hz,
and scale accordingly (add 10 dB per decade of increased bandwidth).
10. Two equal amplitude tones have a power of +10 dBm, and generate a pair of equal amplitude 3rdorder
intermodulation products at 20 dBm. What is the 2tone, 3rdorder intercept point (IP3) of the system?
b)
+25 dBm
2tone, 3rdorder intermod products increase 3 dB in power for every 1 dB increase in tones that produce them.
That means the intermods increase in power at a rate of 2 dB per 1 dB relative to the tone power. The 2tone,
3rdorder intercept point is defined as the theoretical point where the two original tones and the two 3rdorder
products would have equal power (not possible in real systems due to saturation limits).
If the two
original tones have a power of +10 dBm and the 3rdorder products have a power of 20 dBm, then the intercept
point will be at +10 dBm + [(+10)  (20)]/2 dB = +10 dBm + 15 dB = +25 dBm. 


