Difference between revisions of "Aufgaben:Exercise 2.8: Asymmetrical Channel"
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===Solution=== | ===Solution=== | ||
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− | '''(1)''' | + | '''(1)''' For a cosine-shaped source signal and attenuation of the upper sideband, it holds that: |
:$$ r_{\rm TP}(t) = A_{\rm T} + \frac{A_{\rm N}}{2} \cdot \alpha_{\rm O} \cdot{\rm e}^{{\rm j} \cdot \hspace{0.03cm}\omega_{\rm N}\cdot t} + \frac{A_{\rm N}}{2} \cdot{\rm e}^{-{\rm j} \cdot \hspace{0.03cm}\omega_{\rm N}\cdot t}\hspace{0.05cm}.$$ | :$$ r_{\rm TP}(t) = A_{\rm T} + \frac{A_{\rm N}}{2} \cdot \alpha_{\rm O} \cdot{\rm e}^{{\rm j} \cdot \hspace{0.03cm}\omega_{\rm N}\cdot t} + \frac{A_{\rm N}}{2} \cdot{\rm e}^{-{\rm j} \cdot \hspace{0.03cm}\omega_{\rm N}\cdot t}\hspace{0.05cm}.$$ | ||
− | * | + | *At time $t = 0$ all vectors point in the direction of the real axis. |
− | * | + | *Thus $r_{\rm TP}(t = 0)\hspace{0.15cm}\underline { = 15 \ \rm V}$ can be read from the graph on the exercise page. |
− | '''(2)''' | + | '''(2)''' The carrier amplitude is defined by the center of the ellipse: |
− | * | + | $A_{\rm T}\hspace{0.15cm}\underline { = 10 \ \rm V}$. |
+ | *From the equation given in the first subtask, the amplitude $A_{\rm N}$ can thus also be calculated: | ||
:$$ \frac{A_{\rm N}}{2} \cdot ( 1+ \alpha_0) = r_{\rm TP}(t= 0) - A_{\rm T} = 5 \,{\rm V}\hspace{0.3cm} \Rightarrow \hspace{0.3cm}A_{\rm N} \hspace{0.15cm}\underline {= 8 \,{\rm V}} \hspace{0.05cm}.$$ | :$$ \frac{A_{\rm N}}{2} \cdot ( 1+ \alpha_0) = r_{\rm TP}(t= 0) - A_{\rm T} = 5 \,{\rm V}\hspace{0.3cm} \Rightarrow \hspace{0.3cm}A_{\rm N} \hspace{0.15cm}\underline {= 8 \,{\rm V}} \hspace{0.05cm}.$$ | ||
− | * | + | *The point marked '''(2)''' can be used as a check: |
:$$\frac{A_{\rm N}}{2} \cdot ( 1- \alpha_0) = 3 \,{\rm V}\hspace{0.3cm} \Rightarrow \hspace{0.3cm}A_{\rm N} = 8 \,{\rm V} \hspace{0.05cm}.$$ | :$$\frac{A_{\rm N}}{2} \cdot ( 1- \alpha_0) = 3 \,{\rm V}\hspace{0.3cm} \Rightarrow \hspace{0.3cm}A_{\rm N} = 8 \,{\rm V} \hspace{0.05cm}.$$ | ||
− | '''(3)''' | + | '''(3)''' The necessary time for one cycle t $t_1$ is equal to the period of the source signal, i.e., |
:$$t_1= 1/f_{\rm N} \hspace{0.15cm}\underline {=0.5 \ \rm ms}.$$ | :$$t_1= 1/f_{\rm N} \hspace{0.15cm}\underline {=0.5 \ \rm ms}.$$ | ||
− | '''(4)''' | + | '''(4)''' Since the lower sideband is larger than the upper sideband, the peak of the pointer composite moves clockwise around the ellipse. |
− | * | + | *Point '''(2)''' is first reached at time $t_2 = 3/4 · t_1\hspace{0.15cm}\underline { = 0.375 \ \rm ms}$ . |
− | [[File:P_ID1039__Mod_A_2_8_e.png|right|frame| | + | [[File:P_ID1039__Mod_A_2_8_e.png|right|frame|Calculation of $t_2$ and $t_3$]] |
− | '''(5)''' | + | '''(5)''' The pointer length at time $t_2$ can be determined with the [https://en.wikipedia.org/wiki/Pythagorean_theorem Pythagorean Theorem] : |
:$$ a(t = t_2) = \sqrt{(10 \,{\rm V})^2 + (3 \,{\rm V})^2}\hspace{0.15cm}\underline { = 10.44 \,{\rm V}}\hspace{0.05cm}.$$ | :$$ a(t = t_2) = \sqrt{(10 \,{\rm V})^2 + (3 \,{\rm V})^2}\hspace{0.15cm}\underline { = 10.44 \,{\rm V}}\hspace{0.05cm}.$$ | ||
− | * | + | *The phase function is: |
:$$\phi(t = t_2) = {\rm arctan} \frac{3 \,{\rm V}}{10 \,{\rm V}} \hspace{0.15cm}\underline {= 16.7^{\circ}}\hspace{0.05cm}.$$ | :$$\phi(t = t_2) = {\rm arctan} \frac{3 \,{\rm V}}{10 \,{\rm V}} \hspace{0.15cm}\underline {= 16.7^{\circ}}\hspace{0.05cm}.$$ | ||
− | * | + | *The maximum phase $ϕ_{\rm max}$ is slightly larger. It occurs (with a positive sign) at time $t_3 < t_2$ when a straight line from the origin is tangent to the ellipse. |
− | * | + | *By setting up the ellipse equation, this point $(x_3$, $y_3)$ can be accurately calculated analytically. |
− | * | + | *From this, the following would hold for the maximum phase: |
+ | : $\phi_{\rm max} = {\rm arctan} \ {y_3}/{x_3} \hspace{0.05cm}.$ | ||
− | '''(6)''' | + | '''(6)''' The distortion factors of second and third ordern can be obtained from the given equation for nbsp; $v(t)$ $($valid for $f_{\rm N} = 2 \ \rm kHz)$ , and are: |
:$$ K_2 = \frac{0.148 \,{\rm V}}{2.424 \,{\rm V}} = 0.061, \hspace{0.3cm} K_3 = \frac{0.056 \,{\rm V}}{2.424 \,{\rm V}} = 0.023 \hspace{0.05cm}.$$ | :$$ K_2 = \frac{0.148 \,{\rm V}}{2.424 \,{\rm V}} = 0.061, \hspace{0.3cm} K_3 = \frac{0.056 \,{\rm V}}{2.424 \,{\rm V}} = 0.023 \hspace{0.05cm}.$$ | ||
− | * | + | *Thus for the total distortion factor we get: |
:$$K = \sqrt{K_2^2 + K_3^2 }\hspace{0.15cm}\underline { \approx 6.6 \%}.$$ | :$$K = \sqrt{K_2^2 + K_3^2 }\hspace{0.15cm}\underline { \approx 6.6 \%}.$$ | ||
− | '''(7)''' | + | '''(7)''' Frot he power of the useful signal and the interference signal, we obtain: |
:$$ P_{v 1} = \frac{(2.424 \,{\rm V})^2}{2} = 2.94 \,{\rm V}^2\hspace{0.05cm},\hspace{0.3cm} P_{\varepsilon} = \frac{(-0.148 \,{\rm V})^2}{2} + \frac{(0.056 \,{\rm V})^2}{2}= 0.0125 \,{\rm V}^2\hspace{0.05cm}$$ | :$$ P_{v 1} = \frac{(2.424 \,{\rm V})^2}{2} = 2.94 \,{\rm V}^2\hspace{0.05cm},\hspace{0.3cm} P_{\varepsilon} = \frac{(-0.148 \,{\rm V})^2}{2} + \frac{(0.056 \,{\rm V})^2}{2}= 0.0125 \,{\rm V}^2\hspace{0.05cm}$$ | ||
− | * | + | *This gives the signal-to-noise power ratio $\rm (SNR)$: |
:$$\rho_{v} = \frac{P_{v 1}}{P_{\varepsilon }}= \frac{(2.94 \,{\rm V})^2}{0.0125 \,{\rm V}^2} \hspace{0.15cm}\underline {\approx 230} = \frac{1}{K^2} \hspace{0.05cm}.$$ | :$$\rho_{v} = \frac{P_{v 1}}{P_{\varepsilon }}= \frac{(2.94 \,{\rm V})^2}{0.0125 \,{\rm V}^2} \hspace{0.15cm}\underline {\approx 230} = \frac{1}{K^2} \hspace{0.05cm}.$$ | ||
− | * | + | *If, on the other hand, the amplitude distortion were also assigned to the error signal, we would arrive at a much smaller $\rm SNR$. |
− | * | + | *When $P_q = A_{\rm N}^2/2 = 8 \ \rm V^2$ and $P_{\varepsilon}\hspace{0.02cm}' = \overline{(v(t)-q(t))^2} = {1}/{2}\cdot ( 4 \,{\rm V} - 2.424 \,{\rm V})^2 + P_{\varepsilon}= 1.254 \,{\rm V}^2$ one would get: |
:$$\rho_{v }\hspace{0.02cm}' = \frac{8 \,{\rm V}^2}{1.254 \,{\rm V}^2} \approx 6.4\hspace{0.05cm}.$$ | :$$\rho_{v }\hspace{0.02cm}' = \frac{8 \,{\rm V}^2}{1.254 \,{\rm V}^2} \approx 6.4\hspace{0.05cm}.$$ | ||
− | '''(8)''' | + | '''(8)''' All calculations are valid regardless of the message frequency $f_{\rm N}$ if the attenuation factor of the upper sideband remains at $α_{\rm O} = 0.25$ . |
− | * | + | *Thus, the same distortion factor $K\hspace{0.15cm}\underline { \approx 6.6 \%}$ is obtained for $f_{\rm N} = 4 \ \rm kHz$ . |
{{ML-Fuß}} | {{ML-Fuß}} | ||
Revision as of 20:56, 20 December 2021
A cosine-shaped source signal $q(t)$ with amplitude $A_{\rm N}$ and frequency $f_{\rm N}$ is DSB amplitude modulated, such that the modulated signal is given by:
- $$ s(t) = \big[ q(t) + A_{\rm T}\big] \cdot \cos(2 \pi \cdot f_{\rm T} \cdot t ) \hspace{0.05cm}.$$
The transmission channel exhibits linear distortions:
- While the lower sideband $($LSB frequency: $f_{\rm T} - f_{\rm N})$ and the carrier are transmitted undistorted,
- the upper sideband $($USB-Frequenz: $f_{\rm T} + f_{\rm N})$ is weighted with the attenuation factor $α_{\rm O} = 0.25$ .
The graph shows the locus curve, i.e., the representation of the equivalent low-pass signal $r_{\rm TP}(t)$ in the complex plane.
Evaluating the signal $r(t)$ with an ideal envelope demodulator, we obtain a sink signal $v(t)$, which can be approximated as follows:
- $$v(t) = 2.424 \,{\rm V} \cdot \cos(\omega_{\rm N} \cdot t ) -0.148 \,{\rm V} \cdot \cos(2\omega_{\rm N} \cdot t )+ 0.056 \,{\rm V} \cdot \cos(3\omega_{\rm N} \cdot t )-\text{ ...}$$
For this measurement, the message frequency $f_{\rm N} = 2 \ \rm kHz$ was used.
In subtask (7) the signal-to-noise power ratio $\rm (SNR)$ should be calculated as follows:
- $$ \rho_{v } = \frac{P_{v 1}}{P_{\varepsilon }} \hspace{0.05cm}.$$
Here, $P_{v1} = α^2 · P_q$ and $P_ε$ denote the "powers" of both signals:
- $$ v_1(t) = 2.424 \,{\rm V} \cdot \cos(\omega_{\rm N} \cdot t )\hspace{0.05cm},$$
- $$ \varepsilon(t) = v(t) - v_1(t) \approx -0.148 \,{\rm V} \cdot \cos(2\omega_{\rm N} \cdot t )+ 0.056 \,{\rm V} \cdot \cos(3\omega_{\rm N} \cdot t ) \hspace{0.05cm}.$$
Hints:
- This exercise belongs to the chapter Envelope Demodulation.
- Particular reference is made to the page Description using the equivalent low-pass signal.
Questions
Solution
- $$ r_{\rm TP}(t) = A_{\rm T} + \frac{A_{\rm N}}{2} \cdot \alpha_{\rm O} \cdot{\rm e}^{{\rm j} \cdot \hspace{0.03cm}\omega_{\rm N}\cdot t} + \frac{A_{\rm N}}{2} \cdot{\rm e}^{-{\rm j} \cdot \hspace{0.03cm}\omega_{\rm N}\cdot t}\hspace{0.05cm}.$$
- At time $t = 0$ all vectors point in the direction of the real axis.
- Thus $r_{\rm TP}(t = 0)\hspace{0.15cm}\underline { = 15 \ \rm V}$ can be read from the graph on the exercise page.
(2) The carrier amplitude is defined by the center of the ellipse:
$A_{\rm T}\hspace{0.15cm}\underline { = 10 \ \rm V}$.
- From the equation given in the first subtask, the amplitude $A_{\rm N}$ can thus also be calculated:
- $$ \frac{A_{\rm N}}{2} \cdot ( 1+ \alpha_0) = r_{\rm TP}(t= 0) - A_{\rm T} = 5 \,{\rm V}\hspace{0.3cm} \Rightarrow \hspace{0.3cm}A_{\rm N} \hspace{0.15cm}\underline {= 8 \,{\rm V}} \hspace{0.05cm}.$$
- The point marked (2) can be used as a check:
- $$\frac{A_{\rm N}}{2} \cdot ( 1- \alpha_0) = 3 \,{\rm V}\hspace{0.3cm} \Rightarrow \hspace{0.3cm}A_{\rm N} = 8 \,{\rm V} \hspace{0.05cm}.$$
(3) The necessary time for one cycle t $t_1$ is equal to the period of the source signal, i.e.,
- $$t_1= 1/f_{\rm N} \hspace{0.15cm}\underline {=0.5 \ \rm ms}.$$
(4) Since the lower sideband is larger than the upper sideband, the peak of the pointer composite moves clockwise around the ellipse.
- Point (2) is first reached at time $t_2 = 3/4 · t_1\hspace{0.15cm}\underline { = 0.375 \ \rm ms}$ .
(5) The pointer length at time $t_2$ can be determined with the Pythagorean Theorem :
- $$ a(t = t_2) = \sqrt{(10 \,{\rm V})^2 + (3 \,{\rm V})^2}\hspace{0.15cm}\underline { = 10.44 \,{\rm V}}\hspace{0.05cm}.$$
- The phase function is:
- $$\phi(t = t_2) = {\rm arctan} \frac{3 \,{\rm V}}{10 \,{\rm V}} \hspace{0.15cm}\underline {= 16.7^{\circ}}\hspace{0.05cm}.$$
- The maximum phase $ϕ_{\rm max}$ is slightly larger. It occurs (with a positive sign) at time $t_3 < t_2$ when a straight line from the origin is tangent to the ellipse.
- By setting up the ellipse equation, this point $(x_3$, $y_3)$ can be accurately calculated analytically.
- From this, the following would hold for the maximum phase:
- $\phi_{\rm max} = {\rm arctan} \ {y_3}/{x_3} \hspace{0.05cm}.$
(6) The distortion factors of second and third ordern can be obtained from the given equation for nbsp; $v(t)$ $($valid for $f_{\rm N} = 2 \ \rm kHz)$ , and are:
- $$ K_2 = \frac{0.148 \,{\rm V}}{2.424 \,{\rm V}} = 0.061, \hspace{0.3cm} K_3 = \frac{0.056 \,{\rm V}}{2.424 \,{\rm V}} = 0.023 \hspace{0.05cm}.$$
- Thus for the total distortion factor we get:
- $$K = \sqrt{K_2^2 + K_3^2 }\hspace{0.15cm}\underline { \approx 6.6 \%}.$$
(7) Frot he power of the useful signal and the interference signal, we obtain:
- $$ P_{v 1} = \frac{(2.424 \,{\rm V})^2}{2} = 2.94 \,{\rm V}^2\hspace{0.05cm},\hspace{0.3cm} P_{\varepsilon} = \frac{(-0.148 \,{\rm V})^2}{2} + \frac{(0.056 \,{\rm V})^2}{2}= 0.0125 \,{\rm V}^2\hspace{0.05cm}$$
- This gives the signal-to-noise power ratio $\rm (SNR)$:
- $$\rho_{v} = \frac{P_{v 1}}{P_{\varepsilon }}= \frac{(2.94 \,{\rm V})^2}{0.0125 \,{\rm V}^2} \hspace{0.15cm}\underline {\approx 230} = \frac{1}{K^2} \hspace{0.05cm}.$$
- If, on the other hand, the amplitude distortion were also assigned to the error signal, we would arrive at a much smaller $\rm SNR$.
- When $P_q = A_{\rm N}^2/2 = 8 \ \rm V^2$ and $P_{\varepsilon}\hspace{0.02cm}' = \overline{(v(t)-q(t))^2} = {1}/{2}\cdot ( 4 \,{\rm V} - 2.424 \,{\rm V})^2 + P_{\varepsilon}= 1.254 \,{\rm V}^2$ one would get:
- $$\rho_{v }\hspace{0.02cm}' = \frac{8 \,{\rm V}^2}{1.254 \,{\rm V}^2} \approx 6.4\hspace{0.05cm}.$$
(8) All calculations are valid regardless of the message frequency $f_{\rm N}$ if the attenuation factor of the upper sideband remains at $α_{\rm O} = 0.25$ .
- Thus, the same distortion factor $K\hspace{0.15cm}\underline { \approx 6.6 \%}$ is obtained for $f_{\rm N} = 4 \ \rm kHz$ .