Difference between revisions of "Aufgaben:Exercise 2.6Z: Signal-to-Noise Ratio"
(19 intermediate revisions by 4 users not shown) | |||
Line 3: | Line 3: | ||
}} | }} | ||
− | [[File:P_ID1017__Mod_Z_2_6.png|right|frame| | + | [[File:P_ID1017__Mod_Z_2_6.png|right|frame|Spectra and power density spectra]] |
− | + | In the following exercise, we assume: | |
− | * | + | *a cosine source signal: |
:$$ q(t) = 4 \,{\rm V} \cdot \cos(2 \pi \cdot 5\,{\rm kHz} \cdot t )\hspace{0.05cm},$$ | :$$ q(t) = 4 \,{\rm V} \cdot \cos(2 \pi \cdot 5\,{\rm kHz} \cdot t )\hspace{0.05cm},$$ | ||
− | * | + | * DSB–AM by multiplication with |
:$$z(t) = 1 \cdot \cos(2 \pi \cdot 20\,{\rm kHz} \cdot t )\hspace{0.05cm},$$ | :$$z(t) = 1 \cdot \cos(2 \pi \cdot 20\,{\rm kHz} \cdot t )\hspace{0.05cm},$$ | ||
− | * | + | * a frequency-independent attenuation on the channel corresponding to $α_{\rm K} = 10^{–4}$, |
− | * | + | * additive white input noise with power density $N_0 = 4 · 10^{–19} \ \rm W/Hz$, |
− | * | + | * phase-synchronous and frequency-synchronous demodulation by multiplication the same $z(t)$ as at the transmitter, |
− | * | + | * a rectangular low-pass at the synchronous demodulator with cutoff frequency $f_{\rm E} = 5 \ \rm kHz$. |
− | In | + | In the graph, these specifications are shown in the spectral domain. It should be explicitly mentioned that the power-spectral density ${\it Φ}_z(f)$ of the cosine oscillation $z(t)$ is composed of two Dirac delta lines at $±f_{\rm T}$, as in the amplitude spectrum $Z(f)$, but with weight $A^2/4$ instead of $A/2$. The amplitude should always be set to $A=1$ in this exercise. |
− | + | The sink signal $v(t)$ is composed of the useful component $α · q(t)$ and the noise component $ε(t)$ . Thus, the general rule for the signal-to-noise power ratio to be determined is: | |
:$$ \rho_{v } = \frac{\alpha^2 \cdot P_q}{P_\varepsilon}\hspace{0.05cm}.$$ | :$$ \rho_{v } = \frac{\alpha^2 \cdot P_q}{P_\varepsilon}\hspace{0.05cm}.$$ | ||
− | + | This important quality criterion is often abbreviated to $\rm SNR$ ("signal–to–noise power ratio"). | |
− | + | Hints: | |
− | + | *This exercise belongs to the chapter [[Modulation_Methods/Synchronous_Demodulation|Synchronous Demodulation]]. | |
− | + | *Particular reference is made to the pages [[Modulation_Methods/Synchronous_Demodulation#Calculating_noise_power|Calculating noise power]] and [[Modulation_Methods/Synchronous_Demodulation#Relationship_between_the_powers_from_source_signal_and_transmitted signal|Relationship between the powers from source and_transmitted signal]]. | |
− | * | + | *Please note that the variables $α$ and $α_{\rm K}$ need not be the same. |
− | * | + | *All powers refer to a resistance of $R = 50 \ \rm Ω$ with the exception of subtask '''(1)'''. |
− | * | + | *For DSB-AM without carrier, $P_q$ also represents the transmit power $P_{\rm S}$. |
− | * | ||
− | *$P_q$ | ||
− | === | + | ===Questions=== |
<quiz display=simple> | <quiz display=simple> | ||
− | { | + | {Calculate the transmit power with respect to the unit resistance $R = 1 \ \rm Ω$. |
|type="{}"} | |type="{}"} | ||
$P_q \ = \ $ { 8 3% } $\ \rm V^2$ | $P_q \ = \ $ { 8 3% } $\ \rm V^2$ | ||
− | { | + | {What is the power $P_q$ in watts for the resistor $R = 50 \ \rm Ω$? |
|type="{}"} | |type="{}"} | ||
$P_q \ = \ $ { 0.16 3% } $\ \rm W$ | $P_q \ = \ $ { 0.16 3% } $\ \rm W$ | ||
− | { | + | {Which attenuation factor $α$ results for the whole system? |
|type="{}"} | |type="{}"} | ||
$α \ = \ $ { 0.5 3% } $\ \cdot 10^{-4}$ | $α \ = \ $ { 0.5 3% } $\ \cdot 10^{-4}$ | ||
− | { | + | {Calculate the power density of the noise component $ε(t)$ at the output. What is the value when $f = 0$? Let $H_{\rm E}(f = 0) = 1$. |
|type="{}"} | |type="{}"} | ||
${\it Φ}_ε(f = 0) \ = \ $ { 4 3% } $\ \cdot 10^{-19} \ \rm W/Hz$ | ${\it Φ}_ε(f = 0) \ = \ $ { 4 3% } $\ \cdot 10^{-19} \ \rm W/Hz$ | ||
− | { | + | {What is the noise power of the sink signal? |
|type="{}"} | |type="{}"} | ||
$P_ε \ = \ $ { 4 3% } $\ \cdot 10^{-15} \ \rm W$ | $P_ε \ = \ $ { 4 3% } $\ \cdot 10^{-15} \ \rm W$ | ||
− | { | + | {What is the signal-to-noise power ratio (SNR) at the sink? What is the resulting dB value? |
|type="{}"} | |type="{}"} | ||
$ρ_v \ = \ $ { 100000 3% } | $ρ_v \ = \ $ { 100000 3% } | ||
Line 69: | Line 67: | ||
</quiz> | </quiz> | ||
− | === | + | ===Solution=== |
{{ML-Kopf}} | {{ML-Kopf}} | ||
− | '''(1)''' | + | '''(1)''' The power-spectral density of a cosine signal with amplitude $A$ consists of two Dirac delta lines, each with weight $A^2/4$. |
+ | *The power is obtained from the integral over the PDS and is thus equal to the sum of the two Dirac weights. | ||
+ | *Thus, when $A = 4 \ \rm V$, we obtain the power of the source signal: | ||
:$$ P_q = \frac{A^2}{2} \hspace{0.15cm}\underline {= 8\,{\rm V^2}} \hspace{0.05cm}.$$ | :$$ P_q = \frac{A^2}{2} \hspace{0.15cm}\underline {= 8\,{\rm V^2}} \hspace{0.05cm}.$$ | ||
− | + | *For the modulation method "DSB-AM without a carrier", this is also the transmit power $P_{\rm S}$ in reference to the unit resistance $1\ \rm Ω$. | |
− | '''(2)''' | + | |
+ | |||
+ | '''(2)''' According to the elementary laws of Electrical Engineering: | ||
:$$P_q = \frac{8\,{\rm V^2}}{50\,{\Omega}} \hspace{0.15cm}\underline {= 0.16\,{\rm W}} \hspace{0.05cm}.$$ | :$$P_q = \frac{8\,{\rm V^2}}{50\,{\Omega}} \hspace{0.15cm}\underline {= 0.16\,{\rm W}} \hspace{0.05cm}.$$ | ||
− | |||
− | |||
− | |||
− | |||
− | |||
− | '''( | + | '''(3)''' In the theory section, it is shown that $v(t) = q(t)$ holds under ideal conditions. However, the following should be taken into account: |
− | + | *From the graph, it can be seen that $Z_{\rm E}(f) = Z(f)$ holds. Thus, the receiver-side carrier signal $z_{\rm E}(t)$ has like $z(t)$ the amplitude $1$. | |
− | + | *Ideally, however, the receiver-side carrier signal $z_{\rm E}(t)$ should have amplitude $2$. | |
− | + | *Therefore, $υ(t) = q(t)/2$ applies here. | |
+ | *If we further consider the channel attenuation $α_{\rm K} = 10^{–4}$, we obtain the final result: $α\hspace{0.15cm}\underline { = 0.5 · 10^{–4}}.$ | ||
− | '''(5)''' | + | |
+ | '''(4)''' The power-spectral density of the product $n(t) · z(t)$ is obtained by convolving the two power density spectra of $n(t)$ and $z(t)$: | ||
+ | :$$ {\it \Phi}_\varepsilon \hspace{0.01cm} '(f) = {\it \Phi}_n (f) \star {\it \Phi}_{z }(f)= \frac{N_0}{2} \star \left[\delta(f - f_{\rm T}) + \delta(f + f_{\rm T}) \right]= N_0 \hspace{0.05cm}.$$ | ||
+ | *For the power-spectral density of the signal $ε(t)$ after the low-pass filter, we obtain a rectangular shape with the same value at $f = 0$: | ||
+ | :$${\it \Phi}_\varepsilon (f) = {\it \Phi}_\varepsilon \hspace{0.01cm} '(f) \cdot |H_{\rm E}(f)|^2 \hspace{0.3cm}\Rightarrow \hspace{0.3cm} {\it \Phi}_\varepsilon (f=0)= N_0\hspace{0.15cm}\underline {= 4 \cdot 10^{-19}\,{\rm W/Hz}} \hspace{0.05cm}.$$ | ||
+ | |||
+ | |||
+ | |||
+ | '''(5)''' The noise power is the integral over the noise power density: | ||
:$$ P_{\varepsilon} = \int_{-f_{\rm E}}^{ + f_{\rm E}} {{\it \Phi}_\varepsilon (f)}\hspace{0.1cm}{\rm d}f = N_0 \cdot 2 f_{\rm E} = 4 \cdot 10^{-19}\,\frac{ \rm W}{\rm Hz} \cdot 10^{4}\,{\rm Hz} \hspace{0.15cm}\underline {= 4 \cdot 10^{-15}\,{\rm W}}\hspace{0.05cm}.$$ | :$$ P_{\varepsilon} = \int_{-f_{\rm E}}^{ + f_{\rm E}} {{\it \Phi}_\varepsilon (f)}\hspace{0.1cm}{\rm d}f = N_0 \cdot 2 f_{\rm E} = 4 \cdot 10^{-19}\,\frac{ \rm W}{\rm Hz} \cdot 10^{4}\,{\rm Hz} \hspace{0.15cm}\underline {= 4 \cdot 10^{-15}\,{\rm W}}\hspace{0.05cm}.$$ | ||
− | '''(6)''' | + | |
+ | '''(6)''' From the results of subtasks '''(2)''', '''(3)''' and '''(5)''' it follows that: | ||
:$$\rho_{v } = \frac{\alpha^2 \cdot P_q}{P_\varepsilon} = \frac{(0.5 \cdot 10^{-4})^2 \cdot 0.16\,{\rm W}}{4 \cdot 10^{-15}\,{\rm W}} \hspace{0.15cm}\underline {= 100000} \hspace{0.3cm}\Rightarrow \hspace{0.3cm}10 \cdot {\rm lg }\hspace{0.1cm}\rho_{v } \hspace{0.15cm}\underline {= 50\,{\rm dB}}\hspace{0.05cm}.$$ | :$$\rho_{v } = \frac{\alpha^2 \cdot P_q}{P_\varepsilon} = \frac{(0.5 \cdot 10^{-4})^2 \cdot 0.16\,{\rm W}}{4 \cdot 10^{-15}\,{\rm W}} \hspace{0.15cm}\underline {= 100000} \hspace{0.3cm}\Rightarrow \hspace{0.3cm}10 \cdot {\rm lg }\hspace{0.1cm}\rho_{v } \hspace{0.15cm}\underline {= 50\,{\rm dB}}\hspace{0.05cm}.$$ | ||
Line 102: | Line 109: | ||
− | [[Category: | + | [[Category:Modulation Methods: Exercises|^2.2 Synchronous Demodulation^]] |
Latest revision as of 15:19, 18 January 2023
In the following exercise, we assume:
- a cosine source signal:
- $$ q(t) = 4 \,{\rm V} \cdot \cos(2 \pi \cdot 5\,{\rm kHz} \cdot t )\hspace{0.05cm},$$
- DSB–AM by multiplication with
- $$z(t) = 1 \cdot \cos(2 \pi \cdot 20\,{\rm kHz} \cdot t )\hspace{0.05cm},$$
- a frequency-independent attenuation on the channel corresponding to $α_{\rm K} = 10^{–4}$,
- additive white input noise with power density $N_0 = 4 · 10^{–19} \ \rm W/Hz$,
- phase-synchronous and frequency-synchronous demodulation by multiplication the same $z(t)$ as at the transmitter,
- a rectangular low-pass at the synchronous demodulator with cutoff frequency $f_{\rm E} = 5 \ \rm kHz$.
In the graph, these specifications are shown in the spectral domain. It should be explicitly mentioned that the power-spectral density ${\it Φ}_z(f)$ of the cosine oscillation $z(t)$ is composed of two Dirac delta lines at $±f_{\rm T}$, as in the amplitude spectrum $Z(f)$, but with weight $A^2/4$ instead of $A/2$. The amplitude should always be set to $A=1$ in this exercise.
The sink signal $v(t)$ is composed of the useful component $α · q(t)$ and the noise component $ε(t)$ . Thus, the general rule for the signal-to-noise power ratio to be determined is:
- $$ \rho_{v } = \frac{\alpha^2 \cdot P_q}{P_\varepsilon}\hspace{0.05cm}.$$
This important quality criterion is often abbreviated to $\rm SNR$ ("signal–to–noise power ratio").
Hints:
- This exercise belongs to the chapter Synchronous Demodulation.
- Particular reference is made to the pages Calculating noise power and Relationship between the powers from source and_transmitted signal.
- Please note that the variables $α$ and $α_{\rm K}$ need not be the same.
- All powers refer to a resistance of $R = 50 \ \rm Ω$ with the exception of subtask (1).
- For DSB-AM without carrier, $P_q$ also represents the transmit power $P_{\rm S}$.
Questions
Solution
- The power is obtained from the integral over the PDS and is thus equal to the sum of the two Dirac weights.
- Thus, when $A = 4 \ \rm V$, we obtain the power of the source signal:
- $$ P_q = \frac{A^2}{2} \hspace{0.15cm}\underline {= 8\,{\rm V^2}} \hspace{0.05cm}.$$
- For the modulation method "DSB-AM without a carrier", this is also the transmit power $P_{\rm S}$ in reference to the unit resistance $1\ \rm Ω$.
(2) According to the elementary laws of Electrical Engineering:
- $$P_q = \frac{8\,{\rm V^2}}{50\,{\Omega}} \hspace{0.15cm}\underline {= 0.16\,{\rm W}} \hspace{0.05cm}.$$
(3) In the theory section, it is shown that $v(t) = q(t)$ holds under ideal conditions. However, the following should be taken into account:
- From the graph, it can be seen that $Z_{\rm E}(f) = Z(f)$ holds. Thus, the receiver-side carrier signal $z_{\rm E}(t)$ has like $z(t)$ the amplitude $1$.
- Ideally, however, the receiver-side carrier signal $z_{\rm E}(t)$ should have amplitude $2$.
- Therefore, $υ(t) = q(t)/2$ applies here.
- If we further consider the channel attenuation $α_{\rm K} = 10^{–4}$, we obtain the final result: $α\hspace{0.15cm}\underline { = 0.5 · 10^{–4}}.$
(4) The power-spectral density of the product $n(t) · z(t)$ is obtained by convolving the two power density spectra of $n(t)$ and $z(t)$:
- $$ {\it \Phi}_\varepsilon \hspace{0.01cm} '(f) = {\it \Phi}_n (f) \star {\it \Phi}_{z }(f)= \frac{N_0}{2} \star \left[\delta(f - f_{\rm T}) + \delta(f + f_{\rm T}) \right]= N_0 \hspace{0.05cm}.$$
- For the power-spectral density of the signal $ε(t)$ after the low-pass filter, we obtain a rectangular shape with the same value at $f = 0$:
- $${\it \Phi}_\varepsilon (f) = {\it \Phi}_\varepsilon \hspace{0.01cm} '(f) \cdot |H_{\rm E}(f)|^2 \hspace{0.3cm}\Rightarrow \hspace{0.3cm} {\it \Phi}_\varepsilon (f=0)= N_0\hspace{0.15cm}\underline {= 4 \cdot 10^{-19}\,{\rm W/Hz}} \hspace{0.05cm}.$$
(5) The noise power is the integral over the noise power density:
- $$ P_{\varepsilon} = \int_{-f_{\rm E}}^{ + f_{\rm E}} {{\it \Phi}_\varepsilon (f)}\hspace{0.1cm}{\rm d}f = N_0 \cdot 2 f_{\rm E} = 4 \cdot 10^{-19}\,\frac{ \rm W}{\rm Hz} \cdot 10^{4}\,{\rm Hz} \hspace{0.15cm}\underline {= 4 \cdot 10^{-15}\,{\rm W}}\hspace{0.05cm}.$$
(6) From the results of subtasks (2), (3) and (5) it follows that:
- $$\rho_{v } = \frac{\alpha^2 \cdot P_q}{P_\varepsilon} = \frac{(0.5 \cdot 10^{-4})^2 \cdot 0.16\,{\rm W}}{4 \cdot 10^{-15}\,{\rm W}} \hspace{0.15cm}\underline {= 100000} \hspace{0.3cm}\Rightarrow \hspace{0.3cm}10 \cdot {\rm lg }\hspace{0.1cm}\rho_{v } \hspace{0.15cm}\underline {= 50\,{\rm dB}}\hspace{0.05cm}.$$