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This module gives an introduction to the continuous time impulse response of LTI systems.

Introduction

  • The output of an LTI system is completely determined by the input and the system's response to a unit impulse.

    System output

    A continuous time system H takes the input f(t) and produces the output y(t).
    We can determine the system's output, y(t), if we know the system's impulse response, h(t), and the input, f(t).
  • The output for a unit impulse input is called the impulse response.
    An impulse input delta(t) going through a continuous time system H, producing the system's impulse response, h(t). delta(t) 'shocks' the system suddenly and h(t) is the response to the shock.

Example approximate impulses

  1. Hammer blow to a structure
  2. Hand clap or gun blast in a room
  3. Air gun blast underwater

Lti systems and impulse responses

Finding system outputs

By the sifting property of impulses, any signal can be decomposed in terms of an integral of shifted, scaled impulses.

f t τ f τ δ t τ

δ t τ peaks up where t τ .

The functions δ(t-τ) and f(τ) as functions of τ. δ(t-τ) is a peak of infinite height and zero width at point t. f(τ) is some function with a strange shape. Point t is marked on the graphs of both of them.

Since we know the response of the system to an impulse and any signal can be decomposed into impulses, all we need to do to find the response of the system to any signal is to decompose the signal into impulses, calculate the system's output for every impulse and add the outputs back together. This is the process known as Convolution . Since we are in Continuous Time , this is the Continuous Time Convolution Integral .

Finding impulse responses

  • Theory:
    1. Solve the system's differential equation for y(t) with f t δ t
    2. Use the Laplace transform
  • Practice:
    1. Apply an impulse-like input signal to the system and measure the output
    2. Use Fourier methods
  • We will assume that h(t) is given for now.
    • The goal now is to compute the output y(t) given the impulse response h(t) and the input f(t).
      A system with impulse response h takes the input f and produces the output y.

Impulse response summary

When a system is "shocked" by a delta function, it produces an output known as its impulse response. For an LTI system, the impulse response completely determines the output of the system given any arbitrary input. The output can be found using continuous time convolution.

Questions & Answers

how does the planets on our solar system orbit
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Astronomy (from Ancient Greek ἀστρονομία (astronomía) 'science that studies the laws of the stars') is a natural science that studies celestial objects and phenomena. It uses mathematics, physics, and chemistry in order to explain their origin and evolution.
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solar Univers
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GANGAIN Reply
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GANGAIN
Comets are cosmic snowballs of frozen gases , rock and dust that orbit the sun. They are mostly found between the orbits of Venus and Mercury.
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sahil
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Govinda Reply
why the moon is always appear in an elliptical shape
Gatjuol Reply
Because when astroid hit the Earth then a piece of elliptical shape of the earth was separated which is now called moon.
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lidiya Reply
Did you mean eye sight or sea level
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according to the theory of astronomers why the moon is always appear in an elliptical orbit?
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hi !!! I am new in astronomy.... I have so many questions in mind .... all of scientists of the word they just give opinion only. but they never think true or false ... i respect all of them... I believes whole universe depending on true ...থিউরি
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there many theory to born universe but what is the reality of big bang theory to born universe
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universal
there are many theories regarding this it's on you believe any theory that you think is true ex. eternal inflation theory, oscillation model theory, multiple universe theory the big bang theory etc.
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I think it couldn't possible on earth
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is that so. the question was in the end of this chapter
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in theory, you could see them all from the equator (though over the course of a year, not at pne time). stars are measured in "declination", which is how far N or S of the equator (90* to -90*). Polaris is the North star, and is ALMOST 90* (+89*). So it would just barely creep over the horizon.
Christopher
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Source:  OpenStax, Signals and systems. OpenStax CNX. Aug 14, 2014 Download for free at http://legacy.cnx.org/content/col10064/1.15
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