Signals and Systems - Quick Guide



What is Signal?

Signal is a time varying physical phenomenon which is intended to convey information.

OR

Signal is a function of time.

OR

Signal is a function of one or more independent variables, which contain some information.

Example: voice signal, video signal, signals on telephone wires etc.

Note: Noise is also a signal, but the information conveyed by noise is unwanted hence it is considered as undesirable.

signal overview

What is System?

System is a device or combination of devices, which can operate on signals and produces corresponding response. Input to a system is called as excitation and output from it is called as response.

For one or more inputs, the system can have one or more outputs.

Example: Communication System

signal system

Signals Basic Types

Here are a few basic signals:

Unit Step Function

Unit step function is denoted by u(t). It is defined as u(t) = $\left\{\begin{matrix}1 & t \geqslant 0\\ 0 & t<0 \end{matrix}\right.$

Unit Step Function
  • It is used as best test signal.
  • Area under unit step function is unity.

Unit Impulse Function

Impulse function is denoted by δ(t). and it is defined as δ(t) = $\left\{\begin{matrix}1 & t = 0\\ 0 & t\neq 0 \end{matrix}\right.$

Unit Impulse Function

$$ \int_{-\infty}^{\infty} δ(t)dt=u (t)$$

$$ \delta(t) = {du(t) \over dt } $$

Ramp Signal

Ramp signal is denoted by r(t), and it is defined as r(t) = $\left\{\begin {matrix}t & t\geqslant 0\\ 0 & t < 0 \end{matrix}\right. $

Ramp Signal

$$ \int u(t) = \int 1 = t = r(t) $$

$$ u(t) = {dr(t) \over dt} $$

Area under unit ramp is unity.

Parabolic Signal

Parabolic signal can be defined as x(t) = $\left\{\begin{matrix} t^2/2 & t \geqslant 0\\ 0 & t < 0 \end{matrix}\right.$

Parabolic Signal

$$\iint u(t)dt = \int r(t)dt = \int t dt = {t^2 \over 2} = parabolic signal $$

$$ \Rightarrow u(t) = {d^2x(t) \over dt^2} $$

$$ \Rightarrow r(t) = {dx(t) \over dt} $$

Signum Function

Signum function is denoted as sgn(t). It is defined as sgn(t) = $ \left\{\begin{matrix}1 & t>0\\ 0 & t=0\\ -1 & t<0 \end{matrix}\right. $

Signum Function
sgn(t) = 2u(t) 1

Exponential Signal

Exponential signal is in the form of x(t) = $e^{\alpha t}$.

The shape of exponential can be defined by $\alpha$.

Case i: if $\alpha$ = 0 $\to$ x(t) = $e^0$ = 1

Exponential signal

Case ii: if $\alpha$ < 0 i.e. -ve then x(t) = $e^{-\alpha t}$. The shape is called decaying exponential.

Exponential signal

Case iii: if $\alpha$ > 0 i.e. +ve then x(t) = $e^{\alpha t}$. The shape is called raising exponential.

Exponential signal

Rectangular Signal

Let it be denoted as x(t) and it is defined as

Rectangular signal

Triangular Signal

Let it be denoted as x(t)

Triangular signal

Sinusoidal Signal

Sinusoidal signal is in the form of x(t) = A cos(${w}_{0}\,\pm \phi$) or A sin(${w}_{0}\,\pm \phi$)

Sinusoidal signal

Where T0 = $ 2\pi \over {w}_{0} $

Sinc Function

It is denoted as sinc(t) and it is defined as sinc

$$ (t) = {sin \pi t \over \pi t} $$

$$ = 0\, \text{for t} = \pm 1, \pm 2, \pm 3 ... $$

Sinc Function

Sampling Function

It is denoted as sa(t) and it is defined as

$$sa(t) = {sin t \over t}$$

$$= 0 \,\, \text{for t} = \pm \pi,\, \pm 2 \pi,\, \pm 3 \pi \,... $$

Sampling Function

Signals Classification

Signals are classified into the following categories:

  • Continuous Time and Discrete Time Signals

  • Deterministic and Non-deterministic Signals

  • Even and Odd Signals

  • Periodic and Aperiodic Signals

  • Energy and Power Signals

  • Real and Imaginary Signals

Continuous Time and Discrete Time Signals

A signal is said to be continuous when it is defined for all instants of time.

Continuous signal

A signal is said to be discrete when it is defined at only discrete instants of time/

Discrete signal

Deterministic and Non-deterministic Signals

A signal is said to be deterministic if there is no uncertainty with respect to its value at any instant of time. Or, signals which can be defined exactly by a mathematical formula are known as deterministic signals.

Deterministic signal

A signal is said to be non-deterministic if there is uncertainty with respect to its value at some instant of time. Non-deterministic signals are random in nature hence they are called random signals. Random signals cannot be described by a mathematical equation. They are modelled in probabilistic terms.

Non-deterministic signal

Even and Odd Signals

A signal is said to be even when it satisfies the condition x(t) = x(-t)

Example 1: t2, t4 cost etc.

    Let x(t) = t2

    x(-t) = (-t)2 = t2 = x(t)

    $\therefore, $ t2 is even function

Example 2: As shown in the following diagram, rectangle function x(t) = x(-t) so it is also even function.

Even and odd signals

A signal is said to be odd when it satisfies the condition x(t) = -x(-t)

Example: t, t3 ... And sin t

    Let x(t) = sin t

    x(-t) = sin(-t) = -sin t = -x(t)

    $\therefore, $ sin t is odd function.

Any function ƒ(t) can be expressed as the sum of its even function ƒe(t) and odd function ƒo(t).

    ƒ(t ) = ƒe(t ) + ƒ0(t )

    where

    ƒe(t ) = ½[ƒ(t ) +ƒ(-t )]

Periodic and Aperiodic Signals

A signal is said to be periodic if it satisfies the condition x(t) = x(t + T) or x(n) = x(n + N).

Where

    T = fundamental time period,

    1/T = f = fundamental frequency.

Periodic_and_aperiodic_signals

The above signal will repeat for every time interval T0 hence it is periodic with period T0.

Energy and Power Signals

A signal is said to be energy signal when it has finite energy.

$$\text{Energy}\, E = \int_{-\infty}^{\infty} x^2\,(t)dt$$

A signal is said to be power signal when it has finite power.

$$\text{Power}\, P = \lim_{T \to \infty}\,{1\over2T}\,\int_{-T}^{T}\,x^2(t)dt$$

NOTE:A signal cannot be both, energy and power simultaneously. Also, a signal may be neither energy nor power signal.

    Power of energy signal = 0

    Energy of power signal = ∞

Real and Imaginary Signals

A signal is said to be real when it satisfies the condition x(t) = x*(t)

A signal is said to be odd when it satisfies the condition x(t) = -x*(t)

Example:

    If x(t)= 3 then x*(t)=3*=3 here x(t) is a real signal.

    If x(t)= 3j then x*(t)=3j* = -3j = -x(t) hence x(t) is a odd signal.

Note: For a real signal, imaginary part should be zero. Similarly for an imaginary signal, real part should be zero.

Signals Basic Operations

There are two variable parameters in general:

  1. Amplitude
  2. Time

The following operation can be performed with amplitude:

Amplitude Scaling

C x(t) is a amplitude scaled version of x(t) whose amplitude is scaled by a factor C.

Amplitude scaling

Addition

Addition of two signals is nothing but addition of their corresponding amplitudes. This can be best explained by using the following example:

Amplitude addition

As seen from the diagram above,

    -10 < t < -3 amplitude of z(t) = x1(t) + x2(t) = 0 + 2 = 2

    -3 < t < 3 amplitude of z(t) = x1(t) + x2(t) = 1 + 2 = 3

    3 < t < 10 amplitude of z(t) = x1(t) + x2(t) = 0 + 2 = 2

Subtraction

subtraction of two signals is nothing but subtraction of their corresponding amplitudes. This can be best explained by the following example:

Amplitude subtraction

As seen from the diagram above,

  • -10 < t < -3 amplitude of z (t) = x1(t) - x2(t) = 0 - 2 = -2
  • -3 < t < 3 amplitude of z (t) = x1(t) - x2(t) = 1 - 2 = -1
  • 3 < t < 10 amplitude of z (t) = x1(t) + x2(t) = 0 - 2 = -2

Multiplication

Multiplication of two signals is nothing but multiplication of their corresponding amplitudes. This can be best explained by the following example:

Amplitude multiplication

As seen from the diagram above,

    -10 < t < -3 amplitude of z (t) = x1(t) x2(t) = 0 2 = 0

    -3 < t < 3 amplitude of z (t) = x1(t) x2(t) = 1 2 = 2

    3 < t < 10 amplitude of z (t) = x1(t) x2(t) = 0 2 = 0

The following operations can be performed with time:

Time Shifting

x(t $\pm$ t0) is time shifted version of the signal x(t).

    x (t + t0) $\to$ negative shift

    x (t - t0) $\to$ positive shift

Time shifting

Time Scaling

x(At) is time scaled version of the signal x(t). where A is always positive.

    |A| > 1 $\to$ Compression of the signal

    |A| < 1 $\to$ Expansion of the signal

Time scaling

Note: u(at) = u(t) time scaling is not applicable for unit step function.

Time Reversal

x(-t) is the time reversal of the signal x(t).

Time reversal

Systems Classification

Systems are classified into the following categories:

  • linear and Non-linear Systems
  • Time Variant and Time Invariant Systems
  • linear Time variant and linear Time invariant systems
  • Static and Dynamic Systems
  • Causal and Non-causal Systems
  • Invertible and Non-Invertible Systems
  • Stable and Unstable Systems

linear and Non-linear Systems

A system is said to be linear when it satisfies superposition and homogenate principles. Consider two systems with inputs as x1(t), x2(t), and outputs as y1(t), y2(t) respectively. Then, according to the superposition and homogenate principles,

    T [a1 x1(t) + a2 x2(t)] = a1 T[x1(t)] + a2 T[x2(t)]

    $\therefore, $ T [a1 x1(t) + a2 x2(t)] = a1 y1(t) + a2 y2(t)

From the above expression, is clear that response of overall system is equal to response of individual system.

Example:

    (t) = x2(t)

    Solution:

      y1 (t) = T[x1(t)] = x12(t)

      y2 (t) = T[x2(t)] = x22(t)

      T [a1 x1(t) + a2 x2(t)] = [ a1 x1(t) + a2 x2(t)]2

Which is not equal to a1 y1(t) + a2 y2(t). Hence the system is said to be non linear.

Time Variant and Time Invariant Systems

A system is said to be time variant if its input and output characteristics vary with time. Otherwise, the system is considered as time invariant.

The condition for time invariant system is:

    y (n , t) = y(n-t)

The condition for time variant system is:

    y (n , t) $\neq$ y(n-t)

Where y (n , t) = T[x(n-t)] = input change

    y (n-t) = output change

Example:

    y(n) = x(-n)

    y(n, t) = T[x(n-t)] = x(-n-t)

    y(n-t) = x(-(n-t)) = x(-n + t)

    $\therefore$ y(n, t) y(n-t). Hence, the system is time variant.

linear Time variant (LTV) and linear Time Invariant (LTI) Systems

If a system is both linear and time variant, then it is called linear time variant (LTV) system.

If a system is both linear and time Invariant then that system is called linear time invariant (LTI) system.

Static and Dynamic Systems

Static system is memory-less whereas dynamic system is a memory system.

Example 1: y(t) = 2 x(t)

For present value t=0, the system output is y(0) = 2x(0). Here, the output is only dependent upon present input. Hence the system is memory less or static.

Example 2: y(t) = 2 x(t) + 3 x(t-3)

For present value t=0, the system output is y(0) = 2x(0) + 3x(-3).

Here x(-3) is past value for the present input for which the system requires memory to get this output. Hence, the system is a dynamic system.

Causal and Non-Causal Systems

A system is said to be causal if its output depends upon present and past inputs, and does not depend upon future input.

For non causal system, the output depends upon future inputs also.

Example 1: y(n) = 2 x(t) + 3 x(t-3)

For present value t=1, the system output is y(1) = 2x(1) + 3x(-2).

Here, the system output only depends upon present and past inputs. Hence, the system is causal.

Example 2: y(n) = 2 x(t) + 3 x(t-3) + 6x(t + 3)

For present value t=1, the system output is y(1) = 2x(1) + 3x(-2) + 6x(4) Here, the system output depends upon future input. Hence the system is non-causal system.

Invertible and Non-Invertible systems

A system is said to invertible if the input of the system appears at the output.

Invertible system

    Y(S) = X(S) H1(S) H2(S)

    = X(S) H1(S) $1 \over ( H1(S) )$       Since H2(S) = 1/( H1(S) )

    $\therefore, $ Y(S) = X(S)

    $\to$ y(t) = x(t)

Hence, the system is invertible.

If y(t) $\neq$ x(t), then the system is said to be non-invertible.

Stable and Unstable Systems

The system is said to be stable only when the output is bounded for bounded input. For a bounded input, if the output is unbounded in the system then it is said to be unstable.

Note: For a bounded signal, amplitude is finite.

Example 1: y (t) = x2(t)

Let the input is u(t) (unit step bounded input) then the output y(t) = u2(t) = u(t) = bounded output.

Hence, the system is stable.

Example 2: y (t) = $\int x(t)\, dt$

Let the input is u (t) (unit step bounded input) then the output y(t) = $\int u(t)\, dt$ = ramp signal (unbounded because amplitude of ramp is not finite it goes to infinite when t $\to$ infinite).

Hence, the system is unstable.

Signals Analysis

Analogy Between Vectors and Signals

There is a perfect analogy between vectors and signals.

Vector

A vector contains magnitude and direction. The name of the vector is denoted by bold face type and their magnitude is denoted by light face type.

Example: V is a vector with magnitude V. Consider two vectors V1 and V2 as shown in the following diagram. Let the component of V1 along with V2 is given by C12V2. The component of a vector V1 along with the vector V2 can obtained by taking a perpendicular from the end of V1 to the vector V2 as shown in diagram:

vectors

The vector V1 can be expressed in terms of vector V2

    V1= C12V2 + Ve

    Where Ve is the error vector.

But this is not the only way of expressing vector V1 in terms of V2. The alternate possibilities are:

V1=C1V2+Ve1

V2=C2V2+Ve2

The error signal is minimum for large component value. If C12=0, then two signals are said to be orthogonal.

Dot Product of Two Vectors

    V1 . V2 = V1.V2 cosθ

      θ = Angle between V1 and V2

    V1 . V2 =V2.V1

    The components of V1 alogn V2 = V1 Cos θ = $V1.V2 \over V2$

From the diagram, components of V1 alogn V2 = C 12 V2

$$V_1.V_2 \over V_2 = C_12\,V_2$$

$$ \Rightarrow C_{12} = {V_1.V_2 \over V_2}$$

Signal

The concept of orthogonality can be applied to signals. Let us consider two signals f1(t) and f2(t). Similar to vectors, you can approximate f1(t) in terms of f2(t) as

    f1(t) = C12 f2(t) + fe(t) for (t1 < t < t2)

    $ \Rightarrow $ fe(t) = f1(t) C12 f2(t)

One possible way of minimizing the error is integrating over the interval t1 to t2.

$${1 \over {t_2 - t_1}} \int_{t_1}^{t_2} [f_e (t)] dt$$

$${1 \over {t_2 - t_1}} \int_{t_1}^{t_2} [f_1(t) - C_{12}f_2(t)]dt $$

However, this step also does not reduce the error to appreciable extent. This can be corrected by taking the square of error function.

$\varepsilon = {1 \over {t_2 - t_1}} \int_{t_1}^{t_2} [f_e (t)]^2 dt$

$\Rightarrow {1 \over {t_2 - t_1}} \int_{t_1}^{t_2} [f_e (t) - C_{12}f_2]^2 dt $

Where ε is the mean square value of error signal. The value of C12 which minimizes the error, you need to calculate ${d\varepsilon \over dC_{12} } = 0 $

$\Rightarrow {d \over dC_{12} } [ {1 \over t_2 - t_1 } \int_{t_1}^{t_2} [f_1 (t) - C_{12} f_2 (t)]^2 dt]= 0 $

$\Rightarrow {1 \over {t_2 - t_1}} \int_{t_1}^{t_2} [ {d \over dC_{12} } f_{1}^2(t) - {d \over dC_{12} } 2f_1(t)C_{12}f_2(t)+ {d \over dC_{12} } f_{2}^{2} (t) C_{12}^2 ] dt =0 $

Derivative of the terms which do not have C12 term are zero.

$\Rightarrow \int_{t_1}^{t_2} - 2f_1(t) f_2(t) dt + 2C_{12}\int_{t_1}^{t_2}[f_{2}^{2} (t)]dt = 0 $

If $C_{12} = {{\int_{t_1}^{t_2}f_1(t)f_2(t)dt } \over {\int_{t_1}^{t_2} f_{2}^{2} (t)dt }} $ component is zero, then two signals are said to be orthogonal.

Put C12 = 0 to get condition for orthogonality.

0 = $ {{\int_{t_1}^{t_2}f_1(t)f_2(t)dt } \over {\int_{t_1}^{t_2} f_{2}^{2} (t)dt }} $

$$ \int_{t_1}^{t_2} f_1 (t)f_2(t) dt = 0 $$

Orthogonal Vector Space

A complete set of orthogonal vectors is referred to as orthogonal vector space. Consider a three dimensional vector space as shown below:

Consider a vector A at a point (X1, Y1, Z1). Consider three unit vectors (VX, VY, VZ) in the direction of X, Y, Z axis respectively. Since these unit vectors are mutually orthogonal, it satisfies that

$$V_X. V_X= V_Y. V_Y= V_Z. V_Z = 1 $$

$$V_X. V_Y= V_Y. V_Z= V_Z. V_X = 0 $$

You can write above conditions as

$$V_a . V_b = \left\{ \begin{array}{l l} 1 & \quad a = b \\ 0 & \quad a \neq b \end{array} \right. $$

The vector A can be represented in terms of its components and unit vectors as

$A = X_1 V_X + Y_1 V_Y + Z_1 V_Z................(1) $

Any vectors in this three dimensional space can be represented in terms of these three unit vectors only.

If you consider n dimensional space, then any vector A in that space can be represented as

$ A = X_1 V_X + Y_1 V_Y + Z_1 V_Z+...+ N_1V_N.....(2) $

As the magnitude of unit vectors is unity for any vector A

The component of A along x axis = A.VX

The component of A along Y axis = A.VY

The component of A along Z axis = A.VZ

Similarly, for n dimensional space, the component of A along some G axis

$= A.VG...............(3)$

Substitute equation 2 in equation 3.

$\Rightarrow CG= (X_1 V_X + Y_1 V_Y + Z_1 V_Z +...+G_1 V_G...+ N_1V_N)V_G$

$= X_1 V_X V_G + Y_1 V_Y V_G + Z_1 V_Z V_G +...+ G_1V_G V_G...+ N_1V_N V_G$

$= G_1 \,\,\,\,\, \text{since } V_G V_G=1$

$If V_G V_G \neq 1 \,\,\text{i.e.} V_G V_G= k$

$AV_G = G_1V_G V_G= G_1K$

$G_1 = {(AV_G) \over K}$

Orthogonal Signal Space

Let us consider a set of n mutually orthogonal functions x1(t), x2(t)... xn(t) over the interval t1 to t2. As these functions are orthogonal to each other, any two signals xj(t), xk(t) have to satisfy the orthogonality condition. i.e.

$$\int_{t_1}^{t_2} x_j(t)x_k(t)dt = 0 \,\,\, \text{where}\, j \neq k$$

$$\text{Let} \int_{t_1}^{t_2}x_{k}^{2}(t)dt = k_k $$

Let a function f(t), it can be approximated with this orthogonal signal space by adding the components along mutually orthogonal signals i.e.

    $\,\,\,f(t) = C_1x_1(t) + C_2x_2(t) + ... + C_nx_n(t) + f_e(t) $

    $\quad\quad=\Sigma_{r=1}^{n} C_rx_r (t) $

    $\,\,\,f(t) = f(t) - \Sigma_{r=1}^n C_rx_r (t) $

Mean sqaure error $ \varepsilon = {1 \over t_2 - t_2 } \int_{t_1}^{t_2} [ f_e(t)]^2 dt$

$$ = {1 \over t_2 - t_2 } \int_{t_1}^{t_2} [ f[t] - \sum_{r=1}^{n} C_rx_r(t) ]^2 dt $$

The component which minimizes the mean square error can be found by

$$ {d\varepsilon \over dC_1} = {d\varepsilon \over dC_2} = ... = {d\varepsilon \over dC_k} = 0 $$

Let us consider ${d\varepsilon \over dC_k} = 0 $

$${d \over dC_k}[ {1 \over t_2 - t_1} \int_{t_1}^{t_2} [ f(t) - \Sigma_{r=1}^n C_rx_r(t)]^2 dt] = 0 $$

All terms that do not contain Ck is zero. i.e. in summation, r=k term remains and all other terms are zero.

$$\int_{t_1}^{t_2} - 2 f(t)x_k(t)dt + 2C_k \int_{t_1}^{t_2} [x_k^2 (t)] dt=0 $$

$$\Rightarrow C_k = {{\int_{t_1}^{t_2}f(t)x_k(t)dt} \over {int_{t_1}^{t_2} x_k^2 (t)dt}} $$

$$\Rightarrow \int_{t_1}^{t_2} f(t)x_k(t)dt = C_kK_k $$

Mean Square Error

The average of square of error function fe(t) is called as mean square error. It is denoted by ε (epsilon).

.

$\varepsilon = {1 \over t_2 - t_1 } \int_{t_1}^{t_2} [f_e (t)]^2dt$

$\,\,\,\,= {1 \over t_2 - t_1 } \int_{t_1}^{t_2} [f_e (t) - \Sigma_{r=1}^n C_rx_r(t)]^2 dt $

$\,\,\,\,= {1 \over t_2 - t_1 } [ \int_{t_1}^{t_2} [f_e^2 (t) ]dt + \Sigma_{r=1}^{n} C_r^2 \int_{t_1}^{t_2} x_r^2 (t) dt - 2 \Sigma_{r=1}^{n} C_r \int_{t_1}^{t_2} x_r (t)f(t)dt$

You know that $C_{r}^{2} \int_{t_1}^{t_2} x_r^2 (t)dt = C_r \int_{t_1}^{t_2} x_r (t)f(d)dt = C_r^2 K_r $

$\varepsilon = {1 \over t_2 - t_1 } [ \int_{t_1}^{t_2} [f^2 (t)] dt + \Sigma_{r=1}^{n} C_r^2 K_r - 2 \Sigma_{r=1}^{n} C_r^2 K_r] $

$\,\,\,\,= {1 \over t_2 - t_1 } [\int_{t_1}^{t_2} [f^2 (t)] dt - \Sigma_{r=1}^{n} C_r^2 K_r ] $

$\, \therefore \varepsilon = {1 \over t_2 - t_1 } [\int_{t_1}^{t_2} [f^2 (t)] dt + (C_1^2 K_1 + C_2^2 K_2 + ... + C_n^2 K_n)] $

The above equation is used to evaluate the mean square error.

Closed and Complete Set of Orthogonal Functions

Let us consider a set of n mutually orthogonal functions x1(t), x2(t)...xn(t) over the interval t1 to t2. This is called as closed and complete set when there exist no function f(t) satisfying the condition $\int_{t_1}^{t_2} f(t)x_k(t)dt = 0 $

If this function is satisfying the equation $\int_{t_1}^{t_2} f(t)x_k(t)dt=0 \,\, \text{for}\, k = 1,2,..$ then f(t) is said to be orthogonal to each and every function of orthogonal set. This set is incomplete without f(t). It becomes closed and complete set when f(t) is included.

f(t) can be approximated with this orthogonal set by adding the components along mutually orthogonal signals i.e.

$$f(t) = C_1 x_1(t) + C_2 x_2(t) + ... + C_n x_n(t) + f_e(t) $$

If the infinite series $C_1 x_1(t) + C_2 x_2(t) + ... + C_n x_n(t)$ converges to f(t) then mean square error is zero.

Orthogonality in Complex Functions

If f1(t) and f2(t) are two complex functions, then f1(t) can be expressed in terms of f2(t) as

$f_1(t) = C_{12}f_2(t) \,\,\,\,\,\,\,\,$ ..with negligible error

Where $C_{12} = {{\int_{t_1}^{t_2} f_1(t)f_2^*(t)dt} \over { \int_{t_1}^{t_2} |f_2(t)|^2 dt}} $

Where $f_2^* (t)$ = complex conjugate of f2(t).

If f1(t) and f2(t) are orthogonal then C12 = 0

$$ {\int_{t_1}^{t_2} f_1 (t) f_2^*(t) dt \over \int_{t_1}^{t_2} |f_2 (t) |^2 dt} = 0 $$

$$\Rightarrow \int_{t_1}^{t_2} f_1 (t) f_2^* (dt) = 0$$

The above equation represents orthogonality condition in complex functions.

Fourier Series

Jean Baptiste Joseph Fourier,a French mathematician and a physicist; was born in Auxerre, France. He initialized Fourier series, Fourier transforms and their applications to problems of heat transfer and vibrations. The Fourier series, Fourier transforms and Fourier's Law are named in his honour.

Jean Baptiste Joseph Fourier (21 March 1768 16 May 1830)

Fourier series

To represent any periodic signal x(t), Fourier developed an expression called Fourier series. This is in terms of an infinite sum of sines and cosines or exponentials. Fourier series uses orthoganality condition.

Fourier Series Representation of Continuous Time Periodic Signals

A signal is said to be periodic if it satisfies the condition x (t) = x (t + T) or x (n) = x (n + N).

Where T = fundamental time period,

    ω0= fundamental frequency = 2π/T

There are two basic periodic signals:

$x(t) = \cos\omega_0t$ (sinusoidal) &

$x(t) = e^{j\omega_0 t} $ (complex exponential)

These two signals are periodic with period $T= 2\pi/\omega_0$.

A set of harmonically related complex exponentials can be represented as {$\phi_k (t)$}

$${ \phi_k (t)} = \{ e^{jk\omega_0t}\} = \{ e^{jk({2\pi \over T})t}\} \text{where} \,k = 0 \pm 1, \pm 2 ..n \,\,\,.....(1) $$

All these signals are periodic with period T

According to orthogonal signal space approximation of a function x (t) with n, mutually orthogonal functions is given by

$$x(t) = \sum_{k = - \infty}^{\infty} a_k e^{jk\omega_0t} ..... (2) $$

$$ = \sum_{k = - \infty}^{\infty} a_kk e^{jk\omega_0t} $$

Where $a_k$= Fourier coefficient = coefficient of approximation.

This signal x(t) is also periodic with period T.

Equation 2 represents Fourier series representation of periodic signal x(t).

The term k = 0 is constant.

The term $k = \pm1$ having fundamental frequency $\omega_0$, is called as 1st harmonics.

The term $k = \pm2$ having fundamental frequency $2\omega_0$, is called as 2nd harmonics, and so on...

The term $k = n$ having fundamental frequency $n\omega0$, is called as nth harmonics.

Deriving Fourier Coefficient

We know that $x(t) = \Sigma_{k=- \infty}^{\infty} a_k e^{jk \omega_0 t} ...... (1)$

Multiply $e^{-jn\omega_0 t}$ on both sides. Then

$$ x(t)e^{-jn\omega_0 t} = \sum_{k=- \infty}^{\infty} a_k e^{jk \omega_0 t} . e^{-jn\omega_0 t} $$

Consider integral on both sides.

$$ \int_{0}^{T} x(t) e^{jk \omega_0 t} dt = \int_{0}^{T} \sum_{k=-\infty}^{\infty} a_k e^{jk \omega_0 t} . e^{-jn\omega_0 t}dt $$

$$ \quad \quad \quad \quad \,\, = \int_{0}^{T} \sum_{k=-\infty}^{\infty} a_k e^{j(k-n) \omega_0 t} . dt$$

$$ \int_{0}^{T} x(t) e^{jk \omega_0 t} dt = \sum_{k=-\infty}^{\infty} a_k \int_{0}^{T} e^{j(k-n) \omega_0 t} dt. \,\, ..... (2)$$

by Euler's formula,

$$ \int_{0}^{T} e^{j(k-n) \omega_0 t} dt. = \int_{0}^{T} \cos(k-n)\omega_0 dt + j \int_{0}^{T} \sin(k-n)\omega_0t\,dt$$

$$ \int_{0}^{T} e^{j(k-n) \omega_0 t} dt. = \left\{ \begin{array}{l l} T & \quad k = n \\ 0 & \quad k \neq n \end{array} \right. $$

Hence in equation 2, the integral is zero for all values of k except at k = n. Put k = n in equation 2.

$$\Rightarrow \int_{0}^{T} x(t) e^{-jn\omega_0 t} dt = a_n T $$

$$\Rightarrow a_n = {1 \over T} \int_{0}^{T} e^{-jn\omega_0 t} dt $$

Replace n by k.

$$\Rightarrow a_k = {1 \over T} \int_{0}^{T} e^{-jk\omega_0 t} dt$$

$$\therefore x(t) = \sum_{k=-\infty}^{\infty} a_k e^{j(k-n) \omega_0 t} $$

$$\text{where} a_k = {1 \over T} \int_{0}^{T} e^{-jk\omega_0 t} dt $$

Fourier Series Properties

These are properties of Fourier series:

Linearity Property

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$ & $ y(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{yn}$

then linearity property states that

$ \text{a}\, x(t) + \text{b}\, y(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} \text{a}\, f_{xn} + \text{b}\, f_{yn}$

Time Shifting Property

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$

then time shifting property states that

$x(t-t_0) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} e^{-jn\omega_0 t_0}f_{xn} $

Frequency Shifting Property

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$

then frequency shifting property states that

$e^{jn\omega_0 t_0} . x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{x(n-n_0)} $

Time Reversal Property

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$

then time reversal property states that

If $ x(-t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{-xn}$

Time Scaling Property

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$

then time scaling property states that

If $ x(at) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$

Time scaling property changes frequency components from $\omega_0$ to $a\omega_0$.

Differentiation and Integration Properties

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$

then differentiation property states that

If $ {dx(t)\over dt} \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} jn\omega_0 . f_{xn}$

& integration property states that

If $ \int x(t) dt \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} {f_{xn} \over jn\omega_0} $

Multiplication and Convolution Properties

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$ & $ y(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{yn}$

then multiplication property states that

$ x(t) . y(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} T f_{xn} * f_{yn}$

& convolution property states that

$ x(t) * y(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} T f_{xn} . f_{yn}$

Conjugate and Conjugate Symmetry Properties

If $ x(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f_{xn}$

Then conjugate property states that

$ x*(t) \xleftarrow[\,]{fourier\,series}\xrightarrow[\,]{coefficient} f*_{xn}$

Conjugate symmetry property for real valued time signal states that

$$f*_{xn} = f_{-xn}$$

& Conjugate symmetry property for imaginary valued time signal states that

$$f*_{xn} = -f_{-xn} $$

Fourier Series Types

Trigonometric Fourier Series (TFS)

$\sin n\omega_0 t$ and $\sin m\omega_0 t$ are orthogonal over the interval $(t_0, t_0+{2\pi \over \omega_0})$. So $\sin\omega_0 t,\, \sin 2\omega_0 t$ forms an orthogonal set. This set is not complete without {$\cos n\omega_0 t$ } because this cosine set is also orthogonal to sine set. So to complete this set we must include both cosine and sine terms. Now the complete orthogonal set contains all cosine and sine terms i.e. {$\sin n\omega_0 t,\,\cos n\omega_0 t$ } where n=0, 1, 2...

$\therefore$ Any function x(t) in the interval $(t_0, t_0+{2\pi \over \omega_0})$ can be represented as

$$ x(t) = a_0 \cos0\omega_0 t+ a_1 \cos 1\omega_0 t+ a_2 \cos2 \omega_0 t +...+ a_n \cos n\omega_0 t + ... $$

$$ + b_0 \sin 0\omega_0 t + b_1 \sin 1\omega_0 t +...+ b_n \sin n\omega_0 t + ... $$

$$ = a_0 + a_1 \cos 1\omega_0 t + a_2 \cos 2 \omega_0 t +...+ a_n \cos n\omega_0 t + ...$$

$$ + b_1 \sin 1\omega_0 t +...+ b_n \sin n\omega_0 t + ...$$

$$ \therefore x(t) = a_0 + \sum_{n=1}^{\infty} (a_n \cos n\omega_0 t + b_n \sin n\omega_0 t ) \quad (t_0< t < t_0+T)$$

The above equation represents trigonometric Fourier series representation of x(t).

$$\text{Where} \,a_0 = {\int_{t_0}^{t_0+T} x(t)1 dt \over \int_{t_0}^{t_0+T} 1^2 dt} = {1 \over T} \int_{t_0}^{t_0+T} x(t)dt $$

$$a_n = {\int_{t_0}^{t_0+T} x(t) \cos n\omega_0 t\,dt \over \int_{t_0}^{t_0+T} \cos ^2 n\omega_0 t\, dt}$$

$$b_n = {\int_{t_0}^{t_0+T} x(t) \sin n\omega_0 t\,dt \over \int_{t_0}^{t_0+T} \sin ^2 n\omega_0 t\, dt}$$

$$\text{Here}\, \int_{t_0}^{t_0+T} \cos ^2 n\omega_0 t\, dt = \int_{t_0}^{t_0+T} \sin ^2 n\omega_0 t\, dt = {T\over 2}$$

$$\therefore a_n = {2\over T} \int_{t_0}^{t_0+T} x(t) \cos n\omega_0 t\,dt$$

$$b_n = {2\over T} \int_{t_0}^{t_0+T} x(t) \sin n\omega_0 t\,dt$$

Exponential Fourier Series (EFS)

Consider a set of complex exponential functions $\left\{e^{jn\omega_0 t}\right\} (n=0, \pm1, \pm2...)$ which is orthogonal over the interval $(t_0, t_0+T)$. Where $T={2\pi \over \omega_0}$ . This is a complete set so it is possible to represent any function f(t) as shown below

$ f(t) = F_0 + F_1e^{j\omega_0 t} + F_2e^{j 2\omega_0 t} + ... + F_n e^{j n\omega_0 t} + ...$

$\quad \quad \,\,F_{-1}e^{-j\omega_0 t} + F_{-2}e^{-j 2\omega_0 t} +...+ F_{-n}e^{-j n\omega_0 t}+...$

$$ \therefore f(t) = \sum_{n=-\infty}^{\infty} F_n e^{j n\omega_0 t} \quad \quad (t_0< t < t_0+T) ....... (1) $$

Equation 1 represents exponential Fourier series representation of a signal f(t) over the interval (t0, t0+T). The Fourier coefficient is given as

$$ F_n = {\int_{t_0}^{t_0+T} f(t) (e^{j n\omega_0 t} )^* dt \over \int_{t_0}^{t_0+T} e^{j n\omega_0 t} (e^{j n\omega_0 t} )^* dt} $$

$$ \quad = {\int_{t_0}^{t_0+T} f(t) e^{-j n\omega_0 t} dt \over \int_{t_0}^{t_0+T} e^{-j n\omega_0 t} e^{j n\omega_0 t} dt} $$

$$ \quad \quad \quad \quad \quad \quad \quad \quad \quad \,\, = {\int_{t_0}^{t_0+T} f(t) e^{-j n\omega_0 t} dt \over \int_{t_0}^{t_0+T} 1\, dt} = {1 \over T} \int_{t_0}^{t_0+T} f(t) e^{-j n\omega_0 t} dt $$

$$ \therefore F_n = {1 \over T} \int_{t_0}^{t_0+T} f(t) e^{-j n\omega_0 t} dt $$

Relation Between Trigonometric and Exponential Fourier Series

Consider a periodic signal x(t), the TFS & EFS representations are given below respectively

$ x(t) = a_0 + \Sigma_{n=1}^{\infty}(a_n \cos n\omega_0 t + b_n \sin n\omega_0 t) ... ... (1)$

$ x(t) = \Sigma_{n=-\infty}^{\infty} F_n e^{j n\omega_0 t}$

$\quad \,\,\, = F_0 + F_1e^{j\omega_0 t} + F_2e^{j 2\omega_0 t} + ... + F_n e^{j n\omega_0 t} + ... $

$\quad \quad \quad \quad F_{-1} e^{-j\omega_0 t} + F_{-2}e^{-j 2\omega_0 t} + ... + F_{-n}e^{-j n\omega_0 t} + ... $

$ = F_0 + F_1(\cos \omega_0 t + j \sin\omega_0 t) + F_2(cos 2\omega_0 t + j \sin 2\omega_0 t) + ... + F_n(\cos n\omega_0 t+j \sin n\omega_0 t)+ ... + F_{-1}(\cos\omega_0 t-j \sin\omega_0 t) + F_{-2}(\cos 2\omega_0 t-j \sin 2\omega_0 t) + ... + F_{-n}(\cos n\omega_0 t-j \sin n\omega_0 t) + ... $

$ = F_0 + (F_1+ F_{-1}) \cos\omega_0 t + (F_2+ F_{-2}) \cos2\omega_0 t +...+ j(F_1 - F_{-1}) \sin\omega_0 t + j(F_2 - F_{-2}) \sin2\omega_0 t+... $

$ \therefore x(t) = F_0 + \Sigma_{n=1}^{\infty}( (F_n +F_{-n} ) \cos n\omega_0 t+j(F_n-F_{-n}) \sin n\omega_0 t) ... ... (2) $

Compare equation 1 and 2.

$a_0= F_0$

$a_n=F_n+F_{-n}$

$b_n = j(F_n-F_{-n} )$

Similarly,

$F_n = \frac12 (a_n - jb_n )$

$F_{-n} = \frac12 (a_n + jb_n )$

Fourier Transforms

The main drawback of Fourier series is, it is only applicable to periodic signals. There are some naturally produced signals such as nonperiodic or aperiodic, which we cannot represent using Fourier series. To overcome this shortcoming, Fourier developed a mathematical model to transform signals between time (or spatial) domain to frequency domain & vice versa, which is called 'Fourier transform'.

Fourier transform has many applications in physics and engineering such as analysis of LTI systems, RADAR, astronomy, signal processing etc.

Deriving Fourier transform from Fourier series

Consider a periodic signal f(t) with period T. The complex Fourier series representation of f(t) is given as

$$ f(t) = \sum_{k=-\infty}^{\infty} a_k e^{jk\omega_0 t} $$

$$ \quad \quad \quad \quad \quad = \sum_{k=-\infty}^{\infty} a_k e^{j {2\pi \over T_0} kt} ... ... (1) $$

Let ${1 \over T_0} = \Delta f$, then equation 1 becomes

$f(t) = \sum_{k=-\infty}^{\infty} a_k e^{j2\pi k \Delta ft} ... ... (2) $

but you know that

    $a_k = {1\over T_0} \int_{t_0}^{t_0+T} f(t) e^{-j k\omega_0 t} dt$

Substitute in equation 2.

(2) $ \Rightarrow f(t) = \Sigma_{k=-\infty}^{\infty} {1 \over T_0} \int_{t_0}^{t_0+T} f(t) e^{-j k\omega_0 t} dt\, e^{j2\pi k \Delta ft} $

Let $t_0={T\over2}$

$ = \Sigma_{k=-\infty}^{\infty} [ \int_{-T\over2}^{T\over2} f(t) e^{-j2 \pi k \Delta ft} dt ] \, e^{j2 \pi k \Delta ft}.\Delta f $

In the limit as $T \to \infty, \Delta f$ approaches differential $df, k \Delta f$ becomes a continuous variable $f$, and summation becomes integration

$$ f(t) = lim_{T \to \infty} \left\{ \Sigma_{k=-\infty}^{\infty} [ \int_{-T\over2}^{T\over2} f(t) e^{-j2 \pi k \Delta ft} dt ] \, e^{j2 \pi k \Delta ft}.\Delta f \right\} $$

$$ = \int_{-\infty}^{\infty} [ \int_{-\infty}^{\infty}\,f(t) e^{-j2\pi ft} dt] e^{j2\pi ft} df $$

$$f(t) = \int_{-\infty}^{\infty}\, F[\omega] e^{j\omega t} d \omega$$

$\text{Where}\,F[\omega] = [ \int_{-\infty}^{\infty}\, f(t) e^{-j2 \pi ft} dt]$

Fourier transform of a signal $$f(t) = F[\omega] = [\int_{-\infty}^{\infty}\, f(t) e^{-j\omega t} dt]$$

Inverse Fourier Transform is $$f(t) = \int_{-\infty}^{\infty}\,F[\omega] e^{j\omega t} d \omega$$

Fourier Transform of Basic Functions

Let us go through Fourier Transform of basic functions:

FT of GATE Function

F.T. of Gate System

$$F[\omega] = AT Sa({\omega T \over 2})$$

FT of Impulse Function

$FT [\omega(t) ] = [\int_{- \infty}^{\infty} \delta (t) e^{-j\omega t} dt] $

$\quad \quad \quad \quad = e^{-j\omega t}\, |\, t = 0 $

$\quad \quad \quad \quad = e^{0} = 1 $

$\quad \therefore \delta (\omega) = 1 $

FT of Unit Step Function:

$U(\omega) = \pi \delta (\omega)+1/j\omega$

FT of Exponentials

$ e^{-at}u(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} 1/(a+j)$

$ e^{-at}u(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} 1/(a+j\omega )$

$ e^{-a\,|\,t\,|} \stackrel{\mathrm{F.T}}{\longleftrightarrow} {2a \over {a^2+^2}}$

$ e^{j \omega_0 t} \stackrel{\mathrm{F.T}}{\longleftrightarrow} \delta (\omega - \omega_0)$

FT of Signum Function

$ sgn(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} {2 \over j \omega }$

Conditions for Existence of Fourier Transform

Any function f(t) can be represented by using Fourier transform only when the function satisfies Dirichlets conditions. i.e.

  • The function f(t) has finite number of maxima and minima.

  • There must be finite number of discontinuities in the signal f(t),in the given interval of time.

  • It must be absolutely integrable in the given interval of time i.e.

    $ \int_{-\infty}^{\infty}\, |\, f(t) | \, dt < \infty $

Discrete Time Fourier Transforms (DTFT)

The discrete-time Fourier transform (DTFT) or the Fourier transform of a discretetime sequence x[n] is a representation of the sequence in terms of the complex exponential sequence $e^{j\omega n}$.

The DTFT sequence x[n] is given by

$$ X(\omega) = \Sigma_{n= -\infty}^{\infty} x(n)e^{-j \omega n} \,\, ...\,... (1) $$

Here, X(ω) is a complex function of real frequency variable ω and it can be written as

$$ X(\omega) = X_{re}(\omega) + jX_{img}(\omega) $$

Where Xre(ω), Ximg(ω) are real and imaginary parts of X(ω) respectively.

$$ X_{re}(\omega) = |\, X(\omega) | \cos\theta(\omega) $$

$$ X_{img}(\omega) = |\, X(\omega) | \sin\theta(\omega) $$

$$ |X(\omega) |^2 = |\, X_{re} (\omega) |^2+ |\,X_{im} (\omega) |^2 $$

And X(ω) can also be represented as $ X(\omega) = |\,X(\omega) | e^{j\theta ()} $

Where $\theta(\omega) = arg{X(\omega) } $

$|\,X(\omega) |, \theta(\omega)$ are called magnitude and phase spectrums of X(ω).

Inverse Discrete-Time Fourier Transform

$$ x(n) = { 1 \over 2\pi} \int_{-\pi}^{\pi} X(\omega) e^{j \omega n} d\omega \,\, ...\,... (2)$$

Convergence Condition:

The infinite series in equation 1 may be converges or may not. x(n) is absolutely summable.

$$ \text{when}\,\, \sum_{n=-\infty}^{\infty} |\, x(n)|\, < \infty $$

An absolutely summable sequence has always a finite energy but a finite-energy sequence is not necessarily to be absolutely summable.

Fourier Transforms Properties

Here are the properties of Fourier Transform:

Linearity Property

$\text{If}\,\,x (t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega) $

$ \text{&} \,\, y(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} Y(\omega) $

Then linearity property states that

$a x (t) + b y (t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} a X(\omega) + b Y(\omega) $

Time Shifting Property

$\text{If}\, x(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X (\omega)$

Then Time shifting property states that

$x (t-t_0) \stackrel{\mathrm{F.T}}{\longleftrightarrow} e^{-j\omega t_0 } X(\omega)$

Frequency Shifting Property

$\text{If}\,\, x(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega)$

Then frequency shifting property states that

$e^{j\omega_0 t} . x (t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega - \omega_0)$

Time Reversal Property

$ \text{If}\,\, x(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega)$

Then Time reversal property states that

$ x (-t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(-\omega)$

Time Scaling Property

$ \text{If}\,\, x (t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega) $

Then Time scaling property states that

$ x (at) {1 \over |\,a\,|} X { \omega \over a}$

Differentiation and Integration Properties

$ If \,\, x (t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega)$

Then Differentiation property states that

$ {dx (t) \over dt} \stackrel{\mathrm{F.T}}{\longleftrightarrow} j\omega . X(\omega)$

$ {d^n x (t) \over dt^n } \stackrel{\mathrm{F.T}}{\longleftrightarrow} (j \omega)^n . X(\omega) $

and integration property states that

$ \int x(t) \, dt \stackrel{\mathrm{F.T}}{\longleftrightarrow} {1 \over j \omega} X(\omega) $

$ \iiint ... \int x(t)\, dt \stackrel{\mathrm{F.T}}{\longleftrightarrow} { 1 \over (j\omega)^n} X(\omega) $

Multiplication and Convolution Properties

$ \text{If} \,\, x(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega) $

$ \text{&} \,\,y(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} Y(\omega) $

Then multiplication property states that

$ x(t). y(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} X(\omega)*Y(\omega) $

and convolution property states that

$ x(t) * y(t) \stackrel{\mathrm{F.T}}{\longleftrightarrow} {1 \over 2 \pi} X(\omega).Y(\omega) $

Distortion Less Transmission

Transmission is said to be distortion-less if the input and output have identical wave shapes. i.e., in distortion-less transmission, the input x(t) and output y(t) satisfy the condition:

y (t) = Kx(t - td)

Where td = delay time and

k = constant.

Take Fourier transform on both sides

FT[ y (t)] = FT[Kx(t - td)]

= K FT[x(t - td)]

According to time shifting property,

= KX(w)$e^{-j \omega t_d}$

$ \therefore Y(w) = KX(w)e^{-j \omega t_d}$

Thus, distortionless transmission of a signal x(t) through a system with impulse response h(t) is achieved when

$|H(\omega)| = K \,\, \text{and} \,\,\,\,$ (amplitude response)

$ \Phi (\omega) = -\omega t_d = -2\pi f t_d \,\,\, $ (phase response)

Amplitude Response and Phase Response

A physical transmission system may have amplitude and phase responses as shown below:

amplitude and phase response in physical transmission system

Hilbert Transform

Hilbert transform of a signal x(t) is defined as the transform in which phase angle of all components of the signal is shifted by $\pm \text{90}^o $.

Hilbert transform of x(t) is represented with $\hat{x}(t)$,and it is given by

$$ \hat{x}(t) = { 1 \over \pi } \int_{-\infty}^{\infty} {x(k) \over t-k } dk $$

The inverse Hilbert transform is given by

$$ \hat{x}(t) = { 1 \over \pi } \int_{-\infty}^{\infty} {x(k) \over t-k } dk $$

x(t), $\hat{x}$(t) is called a Hilbert transform pair.

Properties of the Hilbert Transform

A signal x(t) and its Hilbert transform $\hat{x}$(t) have

  • The same amplitude spectrum.

  • The same autocorrelation function.

  • The energy spectral density is same for both x(t) and $\hat{x}$(t).

  • x(t) and $\hat{x}$(t) are orthogonal.

  • The Hilbert transform of $\hat{x}$(t) is -x(t)

  • If Fourier transform exist then Hilbert transform also exists for energy and power signals.

Convolution and Correlation

Convolution

Convolution is a mathematical operation used to express the relation between input and output of an LTI system. It relates input, output and impulse response of an LTI system as

$$ y (t) = x(t) * h(t) $$

Where y (t) = output of LTI

x (t) = input of LTI

h (t) = impulse response of LTI

There are two types of convolutions:

  • Continuous convolution

  • Discrete convolution

Continuous Convolution

continuous convolution

$ y(t) \,\,= x (t) * h (t) $

$= \int_{-\infty}^{\infty} x(\tau) h (t-\tau)d\tau$

(or)

$= \int_{-\infty}^{\infty} x(t - \tau) h (\tau)d\tau $

Discrete Convolution

Discrete convolution

$y(n)\,\,= x (n) * h (n)$

$= \Sigma_{k = - \infty}^{\infty} x(k) h (n-k) $

(or)

$= \Sigma_{k = - \infty}^{\infty} x(n-k) h (k) $

By using convolution we can find zero state response of the system.

Deconvolution

Deconvolution is reverse process to convolution widely used in signal and image processing.

Properties of Convolution

Commutative Property

$ x_1 (t) * x_2 (t) = x_2 (t) * x_1 (t) $

Distributive Property

$ x_1 (t) * [x_2 (t) + x_3 (t) ] = [x_1 (t) * x_2 (t)] + [x_1 (t) * x_3 (t)]$

Associative Property

$x_1 (t) * [x_2 (t) * x_3 (t) ] = [x_1 (t) * x_2 (t)] * x_3 (t) $

Shifting Property

$ x_1 (t) * x_2 (t) = y (t) $

$ x_1 (t) * x_2 (t-t_0) = y (t-t_0) $

$ x_1 (t-t_0) * x_2 (t) = y (t-t_0) $

$ x_1 (t-t_0) * x_2 (t-t_1) = y (t-t_0-t_1) $

Convolution with Impulse

$ x_1 (t) * \delta (t) = x(t) $

$ x_1 (t) * \delta (t- t_0) = x(t-t_0) $

Convolution of Unit Steps

$ u (t) * u (t) = r(t) $

$ u (t-T_1) * u (t-T_2) = r(t-T_1-T_2) $

$ u (n) * u (n) = [n+1] u(n) $

Scaling Property

If $x (t) * h (t) = y (t) $

then $x (a t) * h (a t) = {1 \over |a|} y (a t)$

Differentiation of Output

if $y (t) = x (t) * h (t)$

then $ {dy (t) \over dt} = {dx(t) \over dt} * h (t) $

or

$ {dy (t) \over dt} = x (t) * {dh(t) \over dt}$

Note:

  • Convolution of two causal sequences is causal.

  • Convolution of two anti causal sequences is anti causal.

  • Convolution of two unequal length rectangles results a trapezium.

  • Convolution of two equal length rectangles results a triangle.

  • A function convoluted itself is equal to integration of that function.

Example: You know that $u(t) * u(t) = r(t)$

According to above note, $u(t) * u(t) = \int u(t)dt = \int 1dt = t = r(t)$

Here, you get the result just by integrating $u(t)$.

Limits of Convoluted Signal

If two signals are convoluted then the resulting convoluted signal has following range:

Sum of lower limits < t < sum of upper limits

Ex: find the range of convolution of signals given below

Limits of convoluted signal

Here, we have two rectangles of unequal length to convolute, which results a trapezium.

The range of convoluted signal is:

Sum of lower limits < t < sum of upper limits

$-1+-2 < t < 2+2 $

$-3 < t < 4 $

Hence the result is trapezium with period 7.

Area of Convoluted Signal

The area under convoluted signal is given by $A_y = A_x A_h$

Where Ax = area under input signal

Ah = area under impulse response

Ay = area under output signal

Proof: $y(t) = \int_{-\infty}^{\infty} x(\tau) h (t-\tau)d\tau$

Take integration on both sides

$ \int y(t)dt \,\,\, =\int \int_{-\infty}^{\infty}\, x (\tau) h (t-\tau)d\tau dt $

$ =\int x (\tau) d\tau \int_{-\infty}^{\infty}\, h (t-\tau) dt $

We know that area of any signal is the integration of that signal itself.

$\therefore A_y = A_x\,A_h$

DC Component

DC component of any signal is given by

$\text{DC component}={\text{area of the signal} \over \text{period of the signal}}$

Ex: what is the dc component of the resultant convoluted signal given below?

dc component of the resultant convoluted signal

Here area of x1(t) = length breadth = 1 3 = 3

area of x2(t) = length breadth = 1 4 = 4

area of convoluted signal = area of x1(t) area of x2(t)

= 3 4 = 12

Duration of the convoluted signal = sum of lower limits < t < sum of upper limits

= -1 + -2 < t < 2+2

= -3 < t < 4

Period=7

$\therefore$ Dc component of the convoluted signal = $\text{area of the signal} \over \text{period of the signal}$

Dc component = ${12 \over 7}$

Discrete Convolution

Let us see how to calculate discrete convolution:

i. To calculate discrete linear convolution:

Convolute two sequences x[n] = {a,b,c} & h[n] = [e,f,g]

discrete linear convolution

Convoluted output = [ ea, eb+fa, ec+fb+ga, fc+gb, gc]

Note: if any two sequences have m, n number of samples respectively, then the resulting convoluted sequence will have [m+n-1] samples.

Example: Convolute two sequences x[n] = {1,2,3} & h[n] = {-1,2,2}

discrete linear convolution

Convoluted output y[n] = [ -1, -2+2, -3+4+2, 6+4, 6]

= [-1, 0, 3, 10, 6]

Here x[n] contains 3 samples and h[n] is also having 3 samples so the resulting sequence having 3+3-1 = 5 samples.

ii. To calculate periodic or circular convolution:

Periodic convolution is valid for discrete Fourier transform. To calculate periodic convolution all the samples must be real. Periodic or circular convolution is also called as fast convolution.

If two sequences of length m, n respectively are convoluted using circular convolution then resulting sequence having max [m,n] samples.

Ex: convolute two sequences x[n] = {1,2,3} & h[n] = {-1,2,2} using circular convolution

discrete linear convolution

Normal Convoluted output y[n] = [ -1, -2+2, -3+4+2, 6+4, 6].

= [-1, 0, 3, 10, 6]

Here x[n] contains 3 samples and h[n] also has 3 samples. Hence the resulting sequence obtained by circular convolution must have max[3,3]= 3 samples.

Now to get periodic convolution result, 1st 3 samples [as the period is 3] of normal convolution is same next two samples are added to 1st samples as shown below:

circular convolution result

$\therefore$ Circular convolution result $y[n] = [9\quad 6\quad 3 ]$

Correlation

Correlation is a measure of similarity between two signals. The general formula for correlation is

$$ \int_{-\infty}^{\infty} x_1 (t)x_2 (t-\tau) dt $$

There are two types of correlation:

  • Auto correlation

  • Cros correlation

Auto Correlation Function

It is defined as correlation of a signal with itself. Auto correlation function is a measure of similarity between a signal & its time delayed version. It is represented with R($\tau$).

Consider a signals x(t). The auto correlation function of x(t) with its time delayed version is given by

$$ R_{11} (\tau) = R (\tau) = \int_{-\infty}^{\infty} x(t)x(t-\tau) dt \quad \quad \text{[+ve shift]} $$

$$\quad \quad \quad \quad \quad = \int_{-\infty}^{\infty} x(t)x(t + \tau) dt \quad \quad \text{[-ve shift]} $$

Where $\tau$ = searching or scanning or delay parameter.

If the signal is complex then auto correlation function is given by

$$ R_{11} (\tau) = R (\tau) = \int_{-\infty}^{\infty} x(t)x * (t-\tau) dt \quad \quad \text{[+ve shift]} $$

$$\quad \quad \quad \quad \quad = \int_{-\infty}^{\infty} x(t + \tau)x * (t) dt \quad \quad \text{[-ve shift]} $$

Properties of Auto-correlation Function of Energy Signal

  • Auto correlation exhibits conjugate symmetry i.e. R ($\tau$) = R*(-$\tau$)

  • Auto correlation function of energy signal at origin i.e. at $\tau$=0 is equal to total energy of that signal, which is given as:

    R (0) = E = $ \int_{-\infty}^{\infty}\,|\,x(t)\,|^2\,dt $

  • Auto correlation function $\infty {1 \over \tau} $,

  • Auto correlation function is maximum at $\tau$=0 i.e |R ($\tau$) | ≤ R (0) ∀ $\tau$

  • Auto correlation function and energy spectral densities are Fourier transform pairs. i.e.

    $F.T\,[ R (\tau) ] = \Psi(\omega)$

    $\Psi(\omega) = \int_{-\infty}^{\infty} R (\tau) e^{-j\omega \tau} d \tau$

  • $ R (\tau) = x (\tau)* x(-\tau) $

Auto Correlation Function of Power Signals

The auto correlation function of periodic power signal with period T is given by

$$ R (\tau) = \lim_{T \to \infty} {1\over T} \int_{{-T \over 2}}^{{T \over 2}}\, x(t) x* (t-\tau) dt $$

Properties

  • Auto correlation of power signal exhibits conjugate symmetry i.e. $ R (\tau) = R*(-\tau)$

  • Auto correlation function of power signal at $\tau = 0$ (at origin)is equal to total power of that signal. i.e.

    $R (0)= \rho $

  • Auto correlation function of power signal $\infty {1 \over \tau}$,

  • Auto correlation function of power signal is maximum at $\tau$ = 0 i.e.,

    $ | R (\tau) | \leq R (0)\, \forall \,\tau$

  • Auto correlation function and power spectral densities are Fourier transform pairs. i.e.,

    $F.T[ R (\tau) ] = s(\omega)$

    $s(\omega) = \int_{-\infty}^{\infty} R (\tau) e^{-j\omega \tau} d\tau$

  • $R (\tau) = x (\tau)* x(-\tau) $

Density Spectrum

Let us see density spectrums:

Energy Density Spectrum

Energy density spectrum can be calculated using the formula:

$$ E = \int_{-\infty}^{\infty} |\,x(f)\,|^2 df $$

Power Density Spectrum

Power density spectrum can be calculated by using the formula:

$$P = \Sigma_{n = -\infty}^{\infty}\, |\,C_n |^2 $$

Cross Correlation Function

Cross correlation is the measure of similarity between two different signals.

Consider two signals x1(t) and x2(t). The cross correlation of these two signals $R_{12}(\tau)$ is given by

$$R_{12} (\tau) = \int_{-\infty}^{\infty} x_1 (t)x_2 (t-\tau)\, dt \quad \quad \text{[+ve shift]} $$

$$\quad \quad = \int_{-\infty}^{\infty} x_1 (t+\tau)x_2 (t)\, dt \quad \quad \text{[-ve shift]}$$

If signals are complex then

$$R_{12} (\tau) = \int_{-\infty}^{\infty} x_1 (t)x_2^{*}(t-\tau)\, dt \quad \quad \text{[+ve shift]} $$

$$\quad \quad = \int_{-\infty}^{\infty} x_1 (t+\tau)x_2^{*} (t)\, dt \quad \quad \text{[-ve shift]}$$

$$R_{21} (\tau) = \int_{-\infty}^{\infty} x_2 (t)x_1^{*}(t-\tau)\, dt \quad \quad \text{[+ve shift]} $$

$$\quad \quad = \int_{-\infty}^{\infty} x_2 (t+\tau)x_1^{*} (t)\, dt \quad \quad \text{[-ve shift]}$$

Properties of Cross Correlation Function of Energy and Power Signals

  • Auto correlation exhibits conjugate symmetry i.e. $R_{12} (\tau) = R^*_{21} (-\tau)$.

  • Cross correlation is not commutative like convolution i.e.

    $$ R_{12} (\tau) \neq R_{21} (-\tau) $$

  • If R12(0) = 0 means, if $ \int_{-\infty}^{\infty} x_1 (t) x_2^* (t) dt = 0$, then the two signals are said to be orthogonal.

    For power signal if $ \lim_{T \to \infty} {1\over T} \int_{{-T \over 2}}^{{T \over 2}}\, x(t) x^* (t)\,dt $ then two signals are said to be orthogonal.

  • Cross correlation function corresponds to the multiplication of spectrums of one signal to the complex conjugate of spectrum of another signal. i.e.

    $$ R_{12} (\tau) \leftarrow \rightarrow X_1(\omega) X_2^*(\omega)$$

    This also called as correlation theorem.

Parseval's Theorem

Parseval's theorem for energy signals states that the total energy in a signal can be obtained by the spectrum of the signal as

$ E = {1\over 2 \pi} \int_{-\infty}^{\infty} |X(\omega)|^2 d\omega $

Note: If a signal has energy E then time scaled version of that signal x(at) has energy E/a.

Signals Sampling Theorem

Statement: A continuous time signal can be represented in its samples and can be recovered back when sampling frequency fs is greater than or equal to the twice the highest frequency component of message signal. i. e.

$$ f_s \geq 2 f_m. $$

Proof: Consider a continuous time signal x(t). The spectrum of x(t) is a band limited to fm Hz i.e. the spectrum of x(t) is zero for |ω|>ωm.

Sampling of input signal x(t) can be obtained by multiplying x(t) with an impulse train δ(t) of period Ts. The output of multiplier is a discrete signal called sampled signal which is represented with y(t) in the following diagrams:

Signal Sampling

Here, you can observe that the sampled signal takes the period of impulse. The process of sampling can be explained by the following mathematical expression:

$ \text{Sampled signal}\, y(t) = x(t) . \delta(t) \,\,...\,...(1) $

The trigonometric Fourier series representation of $\delta$(t) is given by

$ \delta(t)= a_0 + \Sigma_{n=1}^{\infty}(a_n \cos n\omega_s t + b_n \sin n\omega_s t )\,\,...\,...(2) $

Where $ a_0 = {1\over T_s} \int_{-T \over 2}^{ T \over 2} \delta (t)dt = {1\over T_s} \delta(0) = {1\over T_s} $

$ a_n = {2 \over T_s} \int_{-T \over 2}^{T \over 2} \delta (t) \cos n\omega_s\, dt = { 2 \over T_2} \delta (0) \cos n \omega_s 0 = {2 \over T}$

$b_n = {2 \over T_s} \int_{-T \over 2}^{T \over 2} \delta(t) \sin n\omega_s t\, dt = {2 \over T_s} \delta(0) \sin n\omega_s 0 = 0 $

Substitute above values in equation 2.

$\therefore\, \delta(t)= {1 \over T_s} + \Sigma_{n=1}^{\infty} ( { 2 \over T_s} \cos n\omega_s t+0)$

Substitute δ(t) in equation 1.

$\to y(t) = x(t) . \delta(t) $

$ = x(t) [{1 \over T_s} + \Sigma_{n=1}^{\infty}({2 \over T_s} \cos n\omega_s t) ] $

$ = {1 \over T_s} [x(t) + 2 \Sigma_{n=1}^{\infty} (\cos n\omega_s t) x(t) ] $

$ y(t) = {1 \over T_s} [x(t) + 2\cos \omega_s t.x(t) + 2 \cos 2\omega_st.x(t) + 2 \cos 3\omega_s t.x(t) \,...\, ...\,] $

Take Fourier transform on both sides.

$Y(\omega) = {1 \over T_s} [X(\omega)+X(\omega-\omega_s )+X(\omega+\omega_s )+X(\omega-2\omega_s )+X(\omega+2\omega_s )+ \,...] $

$\therefore\,\, Y(\omega) = {1\over T_s} \Sigma_{n=-\infty}^{\infty} X(\omega - n\omega_s )\quad\quad where \,\,n= 0,\pm1,\pm2,... $

To reconstruct x(t), you must recover input signal spectrum X(ω) from sampled signal spectrum Y(ω), which is possible when there is no overlapping between the cycles of Y(ω).

Possibility of sampled frequency spectrum with different conditions is given by the following diagrams:

Sampling

Aliasing Effect

The overlapped region in case of under sampling represents aliasing effect, which can be removed by

  • considering fs >2fm

  • By using anti aliasing filters.

Signals Sampling Techniques

There are three types of sampling techniques:

  • Impulse sampling.

  • Natural sampling.

  • Flat Top sampling.

Impulse Sampling

Impulse sampling can be performed by multiplying input signal x(t) with impulse train $\Sigma_{n=-\infty}^{\infty}\delta(t-nT)$ of period 'T'. Here, the amplitude of impulse changes with respect to amplitude of input signal x(t). The output of sampler is given by

Impulse Sampling

$y(t) = x(t) $ impulse train

$= x(t) \Sigma_{n=-\infty}^{\infty} \delta(t-nT)$

$ y(t) = y_{\delta} (t) = \Sigma_{n=-\infty}^{\infty}x(nt) \delta(t-nT)\,...\,... 1 $

To get the spectrum of sampled signal, consider Fourier transform of equation 1 on both sides

$Y(\omega) = {1 \over T} \Sigma_{n=-\infty}^{\infty} X(\omega - n \omega_s ) $

This is called ideal sampling or impulse sampling. You cannot use this practically because pulse width cannot be zero and the generation of impulse train is not possible practically.

Natural Sampling

Natural sampling is similar to impulse sampling, except the impulse train is replaced by pulse train of period T. i.e. you multiply input signal x(t) to pulse train $\Sigma_{n=-\infty}^{\infty} P(t-nT)$ as shown below

Natural Sampling

The output of sampler is

$y(t) = x(t) \times \text{pulse train}$

$= x(t) \times p(t) $

$= x(t) \times \Sigma_{n=-\infty}^{\infty} P(t-nT)\,...\,...(1) $

The exponential Fourier series representation of p(t) can be given as

$p(t) = \Sigma_{n=-\infty}^{\infty} F_n e^{j n\omega_s t}\,...\,...(2) $

$= \Sigma_{n=-\infty}^{\infty} F_n e^{j 2 \pi nf_s t} $

Where $F_n= {1 \over T} \int_{-T \over 2}^{T \over 2} p(t) e^{-j n \omega_s t} dt$

$= {1 \over TP}(n \omega_s)$

Substitute Fn value in equation 2

$ \therefore p(t) = \Sigma_{n=-\infty}^{\infty} {1 \over T} P(n \omega_s)e^{j n \omega_s t}$

$ = {1 \over T} \Sigma_{n=-\infty}^{\infty} P(n \omega_s)e^{j n \omega_s t}$

Substitute p(t) in equation 1

$y(t) = x(t) \times p(t)$

$= x(t) \times {1 \over T} \Sigma_{n=-\infty}^{\infty} P(n \omega_s)\,e^{j n \omega_s t} $

$y(t) = {1 \over T} \Sigma_{n=-\infty}^{\infty} P( n \omega_s)\, x(t)\, e^{j n \omega_s t} $

To get the spectrum of sampled signal, consider the Fourier transform on both sides.

$F.T\, [ y(t)] = F.T [{1 \over T} \Sigma_{n=-\infty}^{\infty} P( n \omega_s)\, x(t)\, e^{j n \omega_s t}]$

$ = {1 \over T} \Sigma_{n=-\infty}^{\infty} P( n \omega_s)\,F.T\,[ x(t)\, e^{j n \omega_s t} ] $

According to frequency shifting property

$F.T\,[ x(t)\, e^{j n \omega_s t} ] = X[\omega-n\omega_s] $

$ \therefore\, Y[\omega] = {1 \over T} \Sigma_{n=-\infty}^{\infty} P( n \omega_s)\,X[\omega-n\omega_s] $

Flat Top Sampling

During transmission, noise is introduced at top of the transmission pulse which can be easily removed if the pulse is in the form of flat top. Here, the top of the samples are flat i.e. they have constant amplitude. Hence, it is called as flat top sampling or practical sampling. Flat top sampling makes use of sample and hold circuit.

Flat top sampling

Theoretically, the sampled signal can be obtained by convolution of rectangular pulse p(t) with ideally sampled signal say yδ(t) as shown in the diagram:

i.e. $ y(t) = p(t) \times y_\delta (t)\, ... \, ...(1) $

Sampled Spectrum

To get the sampled spectrum, consider Fourier transform on both sides for equation 1

$Y[\omega] = F.T\,[P(t) \times y_\delta (t)] $

By the knowledge of convolution property,

$Y[\omega] = P(\omega)\, Y_\delta (\omega)$

Here $P(\omega) = T Sa({\omega T \over 2}) = 2 \sin \omega T/ \omega$

Nyquist Rate

It is the minimum sampling rate at which signal can be converted into samples and can be recovered back without distortion.

Nyquist rate fN = 2fm hz

Nyquist interval = ${1 \over fN}$ = $ {1 \over 2fm}$ seconds.

Samplings of Band Pass Signals

In case of band pass signals, the spectrum of band pass signal X[ω] = 0 for the frequencies outside the range f1 ≤ f ≤ f2. The frequency f1 is always greater than zero. Plus, there is no aliasing effect when fs > 2f2. But it has two disadvantages:

  • The sampling rate is large in proportion with f2. This has practical limitations.

  • The sampled signal spectrum has spectral gaps.

To overcome this, the band pass theorem states that the input signal x(t) can be converted into its samples and can be recovered back without distortion when sampling frequency fs < 2f2.

Also,

$$ f_s = {1 \over T} = {2f_2 \over m} $$

Where m is the largest integer < ${f_2 \over B}$

and B is the bandwidth of the signal. If f2=KB, then

$$ f_s = {1 \over T} = {2KB \over m} $$

For band pass signals of bandwidth 2fm and the minimum sampling rate fs= 2 B = 4fm,

the spectrum of sampled signal is given by $Y[\omega] = {1 \over T} \Sigma_{n=-\infty}^{\infty}\,X[ \omega - 2nB]$

Laplace Transforms (LT)

Complex Fourier transform is also called as Bilateral Laplace Transform. This is used to solve differential equations. Consider an LTI system exited by a complex exponential signal of the form x(t) = Gest.

Where s = any complex number = $\sigma + j\omega$,

σ = real of s, and

ω = imaginary of s

The response of LTI can be obtained by the convolution of input with its impulse response i.e.

$ y(t) = x(t) \times h(t) = \int_{-\infty}^{\infty}\, h (\tau)\, x (t-\tau)d\tau $

$= \int_{-\infty}^{\infty}\, h (\tau)\, Ge^{s(t-\tau)}d\tau $

$= Ge^{st}. \int_{-\infty}^{\infty}\, h (\tau)\, e^{(-s \tau)}d\tau $

$ y(t) = Ge^{st}.H(S) = x(t).H(S)$

Where H(S) = Laplace transform of $h(\tau) = \int_{-\infty}^{\infty} h (\tau) e^{-s\tau} d\tau $

Similarly, Laplace transform of $x(t) = X(S) = \int_{-\infty}^{\infty} x(t) e^{-st} dt\,...\,...(1)$

Relation between Laplace and Fourier transforms

Laplace transform of $x(t) = X(S) =\int_{-\infty}^{\infty} x(t) e^{-st} dt$

Substitute s= σ + jω in above equation.

$ X(\sigma+j\omega) =\int_{-\infty}^{\infty}\,x (t) e^{-(\sigma+j\omega)t} dt$

$ = \int_{-\infty}^{\infty} [ x (t) e^{-\sigma t}] e^{-j\omega t} dt $

$\therefore X(S) = F.T [x (t) e^{-\sigma t}]\,...\,...(2)$

$X(S) = X(\omega) \quad\quad for\,\, s= j\omega$

Inverse Laplace Transform

You know that $X(S) = F.T [x (t) e^{-\sigma t}]$

$\to x (t) e^{-\sigma t} = F.T^{-1} [X(S)] = F.T^{-1} [X(\sigma+j\omega)]$

$= {1\over 2}\pi \int_{-\infty}^{\infty} X(\sigma+j\omega) e^{j\omega t} d\omega$

$ x (t) = e^{\sigma t} {1 \over 2\pi} \int_{-\infty}^{\infty} X(\sigma+j\omega) e^{j\omega t} d\omega $

$= {1 \over 2\pi} \int_{-\infty}^{\infty} X(\sigma+j\omega) e^{(\sigma+j\omega)t} d\omega \,...\,...(3)$

Here, $\sigma+j\omega = s$

$jd = ds d = ds/j$

$ \therefore x (t) = {1 \over 2\pi j} \int_{-\infty}^{\infty} X(s) e^{st} ds\,...\,...(4) $

Equations 1 and 4 represent Laplace and Inverse Laplace Transform of a signal x(t).

Conditions for Existence of Laplace Transform

Dirichlet's conditions are used to define the existence of Laplace transform. i.e.

  • The function f(t) has finite number of maxima and minima.

  • There must be finite number of discontinuities in the signal f(t),in the given interval of time.

  • It must be absolutely integrable in the given interval of time. i.e.

    $ \int_{-\infty}^{\infty} |\,f(t)|\, dt \lt \infty $

Initial and Final Value Theorems

If the Laplace transform of an unknown function x(t) is known, then it is possible to determine the initial and the final values of that unknown signal i.e. x(t) at t=0+ and t=∞.

Initial Value Theorem

Statement: if x(t) and its 1st derivative is Laplace transformable, then the initial value of x(t) is given by

$$ x(0^+) = \lim_{s \to \infty} SX(S) $$

Final Value Theorem

Statement: if x(t) and its 1st derivative is Laplace transformable, then the final value of x(t) is given by

$$ x(\infty) = \lim_{s \to \infty} SX(S) $$

Laplace Transforms Properties

The properties of Laplace transform are:

Linearity Property

If $\,x (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s)$

& $\, y(t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} Y(s)$

Then linearity property states that

$a x (t) + b y (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} a X(s) + b Y(s)$

Time Shifting Property

If $\,x (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s)$

Then time shifting property states that

$x (t-t_0) \stackrel{\mathrm{L.T}}{\longleftrightarrow} e^{-st_0 } X(s)$

Frequency Shifting Property

If $\, x (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s)$

Then frequency shifting property states that

$e^{s_0 t} . x (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s-s_0)$

Time Reversal Property

If $\,x (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s)$

Then time reversal property states that

$x (-t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(-s)$

Time Scaling Property

If $\,x (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s)$

Then time scaling property states that

$x (at) \stackrel{\mathrm{L.T}}{\longleftrightarrow} {1\over |a|} X({s\over a})$

Differentiation and Integration Properties

If $\, x (t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s)$

Then differentiation property states that

$ {dx (t) \over dt} \stackrel{\mathrm{L.T}}{\longleftrightarrow} s. X(s) - s. X(0) $

${d^n x (t) \over dt^n} \stackrel{\mathrm{L.T}}{\longleftrightarrow} (s)^n . X(s)$

The integration property states that

$\int x (t) dt \stackrel{\mathrm{L.T}}{\longleftrightarrow} {1 \over s} X(s)$

$\iiint \,...\, \int x (t) dt \stackrel{\mathrm{L.T}}{\longleftrightarrow} {1 \over s^n} X(s)$

Multiplication and Convolution Properties

If $\,x(t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s)$

and $ y(t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} Y(s)$

Then multiplication property states that

$x(t). y(t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} {1 \over 2 \pi j} X(s)*Y(s)$

The convolution property states that

$x(t) * y(t) \stackrel{\mathrm{L.T}}{\longleftrightarrow} X(s).Y(s)$

Region of Convergence (ROC)

The range variation of for which the Laplace transform converges is called region of convergence.

Properties of ROC of Laplace Transform

  • ROC contains strip lines parallel to jω axis in s-plane.

    strip lines
  • If x(t) is absolutely integral and it is of finite duration, then ROC is entire s-plane.

  • If x(t) is a right sided sequence then ROC : Re{s} > σo.

  • If x(t) is a left sided sequence then ROC : Re{s} < σo.

  • If x(t) is a two sided sequence then ROC is the combination of two regions.

ROC can be explained by making use of examples given below:

Example 1: Find the Laplace transform and ROC of $x(t) = e-^{at}u(t)$

$L.T[x(t)] = L.T[e-^{at}u(t)] = {1 \over S+a}$

$ Re{} \gt -a $

$ ROC:Re{s} \gt >-a$

strip lines

Example 2: Find the Laplace transform and ROC of $x(t) = e^{at}u(-t)$

$ L.T[x(t)] = L.T[e^{at}u(t)] = {1 \over S-a} $

$ Re{s} < a $

$ ROC: Re{s} < a $

strip lines

Example 3: Find the Laplace transform and ROC of $x(t) = e^{-at}u(t)+e^{at}u(-t)$

$L.T[x(t)] = L.T[e^{-at}u(t)+e^{at}u(-t)] = {1 \over S+a} + {1 \over S-a}$

For ${1 \over S+a} Re\{s\} \gt -a $

For ${1 \over S-a} Re\{s\} \lt a $

strip lines

Referring to the above diagram, combination region lies from a to a. Hence,

$ ROC: -a < Re{s} < a $

Causality and Stability

  • For a system to be causal, all poles of its transfer function must be right half of s-plane.

    Casual System
  • A system is said to be stable when all poles of its transfer function lay on the left half of s-plane.

    Stable System
  • A system is said to be unstable when at least one pole of its transfer function is shifted to the right half of s-plane.

    Unstable System
  • A system is said to be marginally stable when at least one pole of its transfer function lies on the jω axis of s-plane.

    Marginally Stable System

ROC of Basic Functions

f(t) F(s) ROC
$u(t)$ $${1\over s}$$ ROC: Re{s} > 0
$ t\, u(t) $ $${1\over s^2} $$ ROC:Re{s} > 0
$ t^n\, u(t) $ $$ {n! \over s^{n+1}} $$ ROC:Re{s} > 0
$ e^{at}\, u(t) $ $$ {1\over s-a} $$ ROC:Re{s} > a
$ e^{-at}\, u(t) $ $$ {1\over s+a} $$ ROC:Re{s} > -a
$ e^{at}\, u(t) $ $$ - {1\over s-a} $$ ROC:Re{s} < a
$ e^{-at}\, u(-t) $ $$ - {1\over s+a} $$ ROC:Re{s} < -a
$ t\, e^{at}\, u(t) $ $$ {1 \over (s-a)^2} $$ ROC:Re{s} > a
$ t^{n} e^{at}\, u(t) $ $$ {n! \over (s-a)^{n+1}} $$ ROC:Re{s} > a
$ t\, e^{-at}\, u(t) $ $$ {1 \over (s+a)^2} $$ ROC:Re{s} > -a
$ t^n\, e^{-at}\, u(t) $ $${n! \over (s+a)^{n+1}} $$ ROC:Re{s} > -a
$ t\, e^{at}\, u(-t) $ $$ - {1 \over (s-a)^2} $$ ROC:Re{s} < a
$ t^n\, e^{at}\, u(-t) $ $$ - {n! \over (s-a)^{n+1}} $$ ROC:Re{s} < a
$ t\, e^{-at}\,u(-t) $ $$ - {1 \over (s+a)^2} $$ ROC:Re{s} < -a
$ t^n\, e^{-at}\, u(-t) $ $$ - {n! \over (s+a)^{n+1}} $$ ROC:Re{s} < -a
$ e^{-at} \cos \, bt $ $$ {s+a \over (s+a)^2 + b^2 } $$
$ e^{-at} \sin\, bt $ $$ {b \over (s+a)^2 + b^2 } $$

Z-Transforms (ZT)

Analysis of continuous time LTI systems can be done using z-transforms. It is a powerful mathematical tool to convert differential equations into algebraic equations.

The bilateral (two sided) z-transform of a discrete time signal x(n) is given as

$Z.T[x(n)] = X(Z) = \Sigma_{n = -\infty}^{\infty} x(n)z^{-n} $

The unilateral (one sided) z-transform of a discrete time signal x(n) is given as

$Z.T[x(n)] = X(Z) = \Sigma_{n = 0}^{\infty} x(n)z^{-n} $

Z-transform may exist for some signals for which Discrete Time Fourier Transform (DTFT) does not exist.

Concept of Z-Transform and Inverse Z-Transform

Z-transform of a discrete time signal x(n) can be represented with X(Z), and it is defined as

$X(Z) = \Sigma_{n=- \infty }^ {\infty} x(n)z^{-n} \,...\,...\,(1)$

If $Z = re^{j\omega}$ then equation 1 becomes

$X(re^{j\omega}) = \Sigma_{n=- \infty}^{\infty} x(n)[re^{j \omega} ]^{-n}$

$= \Sigma_{n=- \infty}^{\infty} x(n)[r^{-n} ] e^{-j \omega n}$

$X(re^{j \omega} ) = X(Z) = F.T[x(n)r^{-n}] \,...\,...\,(2) $

The above equation represents the relation between Fourier transform and Z-transform.

$ X(Z) |_{z=e^{j \omega}} = F.T [x(n)]. $

Inverse Z-transform

$X(re^{j \omega}) = F.T[x(n)r^{-n}] $

$x(n)r^{-n} = F.T^{-1}[X(re^{j \omega}]$

$x(n) = r^n\,F.T^{-1}[X(re^{j \omega} )]$

$= r^n {1 \over 2\pi} \int X(re{^j \omega} )e^{j \omega n} d \omega $

$= {1 \over 2\pi} \int X(re{^j \omega} )[re^{j \omega} ]^n d \omega \,...\,...\,(3)$

Substitute $re^{j \omega} = z$.

$dz = jre^{j \omega} d \omega = jz d \omega$

$d \omega = {1 \over j }z^{-1}dz$

Substitute in equation 3.

$ 3\, \to \, x(n) = {1 \over 2\pi} \int\, X(z)z^n {1 \over j } z^{-1} dz = {1 \over 2\pi j} \int \,X(z) z^{n-1} dz $

$$X(Z) = \sum_{n=- \infty }^{\infty} \,x(n)z^{-n}$$ $$x(n) = {1 \over 2\pi j} \int\, X(z) z^{n-1} dz$$

Z-Transforms Properties

Z-Transform has following properties:

Linearity Property

If $\,x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z)$

and $\,y(n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} Y(Z)$

Then linearity property states that

$a\, x (n) + b\, y (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} a\, X(Z) + b\, Y(Z)$

Time Shifting Property

If $\,x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z)$

Then Time shifting property states that

$x (n-m) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} z^{-m} X(Z)$

Multiplication by Exponential Sequence Property

If $\,x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z)$

Then multiplication by an exponential sequence property states that

$a^n\, . x(n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z/a)$

Time Reversal Property

If $\, x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z)$

Then time reversal property states that

$x (-n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(1/Z)$

Differentiation in Z-Domain OR Multiplication by n Property

If $\, x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z)$

Then multiplication by n or differentiation in z-domain property states that

$ n^k x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} [-1]^k z^k{d^k X(Z) \over dZ^K} $

Convolution Property

If $\,x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z)$

and $\,y(n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} Y(Z)$

Then convolution property states that

$x(n) * y(n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z).Y(Z)$

Correlation Property

If $\,x (n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z)$

and $\,y(n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} Y(Z)$

Then correlation property states that

$x(n) \otimes y(n) \stackrel{\mathrm{Z.T}}{\longleftrightarrow} X(Z).Y(Z^{-1})$

Initial Value and Final Value Theorems

Initial value and final value theorems of z-transform are defined for causal signal.

Initial Value Theorem

For a causal signal x(n), the initial value theorem states that

$ x (0) = \lim_{z \to \infty }X(z) $

This is used to find the initial value of the signal without taking inverse z-transform

Final Value Theorem

For a causal signal x(n), the final value theorem states that

$ x ( \infty ) = \lim_{z \to 1} [z-1] X(z) $

This is used to find the final value of the signal without taking inverse z-transform.

Region of Convergence (ROC) of Z-Transform

The range of variation of z for which z-transform converges is called region of convergence of z-transform.

Properties of ROC of Z-Transforms

  • ROC of z-transform is indicated with circle in z-plane.

  • ROC does not contain any poles.

  • If x(n) is a finite duration causal sequence or right sided sequence, then the ROC is entire z-plane except at z = 0.

  • If x(n) is a finite duration anti-causal sequence or left sided sequence, then the ROC is entire z-plane except at z = ∞.

  • If x(n) is a infinite duration causal sequence, ROC is exterior of the circle with radius a. i.e. |z| > a.

  • If x(n) is a infinite duration anti-causal sequence, ROC is interior of the circle with radius a. i.e. |z| < a.

  • If x(n) is a finite duration two sided sequence, then the ROC is entire z-plane except at z = 0 & z = ∞.

The concept of ROC can be explained by the following example:

Example 1: Find z-transform and ROC of $a^n u[n] + a^{-}nu[-n-1]$

$Z.T[a^n u[n]] + Z.T[a^{-n}u[-n-1]] = {Z \over Z-a} + {Z \over Z {-1 \over a}}$

$$ ROC: |z| \gt a \quad\quad ROC: |z| \lt {1 \over a} $$

The plot of ROC has two conditions as a > 1 and a < 1, as you do not know a.

Unit Circle

In this case, there is no combination ROC.

Unit Circle

Here, the combination of ROC is from $a \lt |z| \lt {1 \over a}$

Hence for this problem, z-transform is possible when a < 1.

Causality and Stability

Causality condition for discrete time LTI systems is as follows:

A discrete time LTI system is causal when

  • ROC is outside the outermost pole.

  • In The transfer function H[Z], the order of numerator cannot be grater than the order of denominator.

Stability Condition for Discrete Time LTI Systems

A discrete time LTI system is stable when

  • its system function H[Z] include unit circle |z|=1.

  • all poles of the transfer function lay inside the unit circle |z|=1.

Z-Transform of Basic Signals

x(t) X[Z]
$\delta$ 1
$u(n)$ ${Z\over Z-1}$
$u(-n-1)$ $ -{Z\over Z-1}$
$\delta(n-m)$ $z^{-m}$
$a^n u[n]$ ${Z \over Z-a}$
$a^n u[-n-1]$ $- {Z \over Z-a}$
$n\,a^n u[n]$ ${aZ \over |Z-a|^2}$
$n\,a^n u[-n-1] $ $- {aZ \over |Z-a|^2}$
$a^n \cos \omega n u[n] $ ${Z^2-aZ \cos \omega \over Z^2-2aZ \cos \omega +a^2}$
$a^n \sin \omega n u[n] $ $ {aZ \sin \omega \over Z^2 -2aZ \cos \omega +a^2 } $
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