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From series to transform

Stretch a pulse train's period until its lines crowd onto one curve, then read that curve, the Fourier transform, by winding, width and band.

Before this5.3 · 7.2 · 4 more
Chapter 8 · Lesson 1 of 4

First, the picture

Repeat a pulse 1 s wide every TT seconds, and let the period grow from 2 s to 16 s, until the pulses hardly ever repeat. Watch the lines of its series crowd together on one dashed curve that never moves.

Period stretch

Unit pulses repeated every T seconds, and their lines, each multiplied by T.

Pulses every 2 s. Each line is multiplied by 2.

period T
2.000 s
line spacing 2π/T
3.142 rad/s
0.00 / 12.00 s
Describe this picture

Two panels. Above, unit pulses repeated every TT, with the period bracketed, such as “T = 2 s”. Below, the lines at kω0k\omega_0, with height “T × c_k (can be negative)” against ω in rad/s, and a dashed curve labelled “fixed curve”. The readouts are “period T” and “line spacing 2π/T”: 2.000 s and 3.142 rad/s at the start. The clip plays once over 12 s, easing between three held frames at periods of 2, 4 and 16 s, where the lines are 3.142, 1.571 and 0.393 rad/s apart. When the clip has finished, dragging along the pulses, or the arrow keys, set the period from 2 s to 16 s; at 6 s the caption reads “Pulses every 6 s: lines 1.047 rad/s apart, on the same curve.”

A signal that does not repeat

A Fourier series needs a wave that repeats. Most signals do not: a single click, one struck bell, one flash of a lamp. This page asks what the lines of 7.2 become when the period is not 1 s or 2 s but infinite, so that nothing ever repeats.

The answer is a curve instead of a row of lines. It is called the Fourier transform, and it describes a signal that happens once. The sums of Fourier series coefficients (7.2) become integrals, and everything else carries over.

I use one signal for the first half of the page: the unit pulse, written rect(t)\mathrm{rect}(t). It is 1 for ∣t∣<12\lvert t\rvert<\tfrac12 and 0 elsewhere, so it is centred on t=0t=0, 1 s wide and 1 high. A pulse of width WW is rect(t/W)\mathrm{rect}(t/W).

Stretch the period: the lines crowd onto one curve

Repeat the unit pulse every TT seconds. Its coefficients are 7.2’s pulse-train formula, ck=1T⋅sin⁡(kω0/2)kω0/2c_k=\tfrac1T\cdot\dfrac{\sin(k\omega_0/2)}{k\omega_0/2}, where ω0=2π/T\omega_0=2\pi/T is the fundamental, in rad/s. For T=2T=2 s the first lines are 0.5, 0.318, 0, −0.1060.5,\ 0.318,\ 0,\ -0.106. For T=8T=8 s they are 0.1250.125, 0.1220.122, 0.1130.113, 0.0980.098, 0.0800.080.

T = 2 sT = 8 s0π2π3πω (rad/s)
Fig. The raw coefficients c_k of a unit pulse repeated every 2 s (top) and every 8 s (bottom), drawn on one frequency axis and one height scale. The lines get closer and shorter.

The lines get closer together and shorter. If they keep shrinking, what is left when TT is infinite? Nothing would be left, which cannot be the answer. The fix is to multiply each line by TT, so I will do that: the quantity I follow from here is T ckT\,c_k.

One thing is new. These pulses are centred, so every ckc_k is a real number. The strips of 7.2 showed only its size ∣ck∣\lvert c_k\rvert, but here the sign stays, so a line can point down.

That is what the picture at the top of the page draws. With pulses every 2 s, each line is multiplied by 2. The lines sit at 0, 3.14, 6.28, 9.420,\ 3.14,\ 6.28,\ 9.42 rad/s, with heights 1, 0.637, 0, −0.2121,\ 0.637,\ 0,\ -0.212.

As the period grows, the pulses move apart and the lines slide along the curve, closer together. With pulses every 4 s there are twice as many lines, on the same curve. They are 1.5711.571 rad/s apart, with heights 11, 0.9000.900, 0.6370.637, 0.3000.300, 00, −0.180-0.180. At 16 s the lines are 0.3930.393 rad/s apart. The curve never moved. Only how closely the lines sit on it changed.

When the clip has finished, drag along the pulses to set the period yourself, from 2 s to 16 s. Think of a camera flash that fires every 2 s, then every 16 s: the flash is the same, and only the gap changes.

Why does the curve stay still? For a pulse that fits inside one period, 7.2’s analysis equation, with the period taken from −T/2-T/2 to T/2T/2, gives

T ck=∫−T/2T/2x(t) e−jkω0t dt.T\,c_k=\int_{-T/2}^{T/2}x(t)\,e^{-jk\omega_0t}\,dt .

Here x(t)x(t) is the single pulse. It is zero outside the period, so the limits can be pushed out to ±∞\pm\infty without changing anything. Now let the frequency kω0k\omega_0 be any number ω\omega and write what is left:

X(jω)=∫−∞∞x(t) e−jωt dt.X(j\omega)=\int_{-\infty}^{\infty}x(t)\,e^{-j\omega t}\,dt .

This is the Fourier transform of xx. The lines of the instrument are the values X(jkω0)X(jk\omega_0), so ck=1TX(jkω0)c_k=\tfrac1T X(jk\omega_0). A longer period only samples the same curve more often.

For a signal that never quite ends, such as a decaying exponential, the lines land on the curve only in the limit T→∞T\to\infty. For a pulse that fits inside one period they are on it for every such TT.

Winding at any rate adds up to X(jω)X(j\omega)

What does the integral mean? 7.2’s machine wound one period of the wave around the origin and took the balance point, which is an average over one period. A single pulse has no period to divide by. So I wind it at any rate ω\omega and add up instead: every instant contributes the point x(t)e−jωtx(t)e^{-j\omega t} times a thin slice of time dtdt, as the strips of Continuous-time convolution (5.3) added up area.

The next instrument is 7.2’s winding panel with a rate that changes continuously, not only in whole laps per period. The unit pulse is wound into an arc, e−jωte^{-j\omega t} for ∣t∣<12\lvert t\rvert<\tfrac12, covering the angles from −ω/2-\omega/2 to +ω/2+\omega/2. Start with the dot, the sum, and watch it as the rate rises.

Winding at any rate: one pulse

A single unit pulse, wound at a rate ω and added up.

No winding: adding up the pulse gives its area, 1.

winding rate ω
0.000 rad/s
sum X(jω)
1.000
0.00 / 12.00 s
Describe this picture

A plane with “real” across and “imaginary” up, holding the wound arc and a dot labelled “sum (signal × s)”. Beside it a strip, “X(jω) (signal × s)”, is traced against ω in rad/s from 0 to 4π4\pi. The readouts are “winding rate ω” and “sum X(jω)”. A sentence under the instrument says why the dot is a sum and not an average. The rate rises from 0, holds at π\pi rad/s, and ends at 4π4\pi rad/s, where the arc is two full circles. Afterwards, dragging along the strip, or the arrow keys, choose the winding rate; at 9.00 rad/s the caption reads “Winding at 9.00 rad/s: it adds up to −0.217.”

With no winding the arc is a single point at 1, and adding up the pulse gives its area, 1. Winding faster, the arc wraps further round the circle, and the strip traces the sum. At π\pi rad/s the arc is half a circle and it adds up to 0.637.

At 4π4\pi rad/s the arc is two full circles. Whole circles add up to 0, and in between the sum swings negative. The strip shows the whole curve, with zeros at 2π2\pi and 4π4\pi rad/s and a dip to −0.217-0.217 near 9 rad/s. Afterwards, drag along the strip to choose your own winding rate. The dot stays on the real axis throughout.

The dot stays on the real axis because the pulse is symmetric about t=0t=0: the arc is a mirror image of itself, so the imaginary parts cancel. A circle that closes adds up to nothing, as in 7.2. A part of a circle adds up to something, and between the zeros it points to the negative side.

Now the integral by hand. For the unit pulse, with ∫eat dt=eat/a\int e^{at}\,dt=e^{at}/a and a=−jωa=-j\omega,

X(jω)=∫−1/21/2e−jωt dt=ejω/2−e−jω/2jω=2sin⁡(ω/2)ω=sin⁡(ω/2)ω/2.X(j\omega)=\int_{-1/2}^{1/2}e^{-j\omega t}\,dt=\frac{e^{j\omega/2}-e^{-j\omega/2}}{j\omega}=\frac{2\sin(\omega/2)}{\omega}=\frac{\sin(\omega/2)}{\omega/2}.

The third step uses a line that is new here, the partner of the cosine rule on Complex exponentials & phasors (3.4): sin⁡θ=ejθ−e−jθ2j\sin\theta=\dfrac{e^{j\theta}-e^{-j\theta}}{2j}, with θ=ω/2\theta=\omega/2. At ω=0\omega=0 the formula reads 0/00/0, and the limit is X(0)=1X(0)=1, the area. At ω=π\omega=\pi it is 2/π=0.6372/\pi=0.637, and at 3π3\pi it is −2/(3π)=−0.212-2/(3\pi)=-0.212.

Two more things to read from this curve. First, the units. A signal in volts, multiplied by seconds, gives volts times seconds, which is why the axes say “signal × s”. A height of XX is therefore an amount per unit of frequency, not an amount at a frequency.

Second, the other direction. Adding up arrows over all frequencies rebuilds the signal:

x(t)=12π∫−∞∞X(jω) ejωt dω.x(t)=\frac1{2\pi}\int_{-\infty}^{\infty}X(j\omega)\,e^{j\omega t}\,d\omega .

This is the inverse transform, and it is 7.2’s synthesis equation with the sum turned into an integral. To see why, write ck=1TX(jkω0)c_k=\tfrac1TX(jk\omega_0) into the synthesis equation, and use 1T=ω02π\tfrac1T=\tfrac{\omega_0}{2\pi}: each term is 12πX(jkω0) ejkω0t⋅ω0\tfrac1{2\pi}X(jk\omega_0)\,e^{jk\omega_0t}\cdot\omega_0, a thin strip of width ω0\omega_0. As TT grows ω0\omega_0 shrinks, the strips become thin, and the sum is the integral, as in 5.3.

The thin strips give a way to read XX: it is a density. The band from ω\omega to ω+Δω\omega+\Delta\omega carries about X(jω) Δω/2πX(j\omega)\,\Delta\omega/2\pi, in the same units as the signal, and a single frequency carries nothing, because a band of zero width has zero area. For the unit pulse, the band from 3.1 to 3.2 rad/s carries about 0.637×0.1/6.283=0.01010.637\times0.1/6.283=0.0101. The mirror band, from −3.2-3.2 to −3.1-3.1, carries the same, and the two arrows turn in opposite directions to make a cosine of height about 0.02020.0202.

Narrower pulse, wider spectrum

Keep the pulse’s area at 1 and squeeze it to width WW, so its height is 1/W1/W. Then the same integral gives

X(jω)=sin⁡(ωW/2)ωW/2.X(j\omega)=\frac{\sin(\omega W/2)}{\omega W/2}.

The height at ω=0\omega=0 stays 1, because it is the area. The curve stretches sideways. Its first zero, the first frequency at which it crosses 0, is at ωW/2=π\omega W/2=\pi, so at 2π/W2\pi/W rad/s. Then width times first zero is 2π2\pi, whatever the width.

In the next instrument the width shrinks from 2 s to 0.125 s. Watch the product of the width and the first zero, not only the picture.

Width and band: squeeze the pulse

A pulse of area 1, squeezed from 2 s to 0.125 s wide, and its spectrum.

A wide pulse: its spectrum is narrow. Width × first zero = 2π.

width
2.000 s
first zero
3.142 rad/s
width × first zero
6.283
0.00 / 8.00 s
Describe this picture

The pulse above, labelled “area 1”, and its spectrum below, “X(jω) (signal × s)” against ω from −60-60 to 6060 rad/s, with triangles at the first zeros. The readouts are “width”, “first zero” and “width × first zero”. The width shrinks from 2 s to 0.125 s, holding at three frames: 2 s, 0.5 s (at 4 s into the clip) and 0.125 s.

A wide pulse has a narrow spectrum. At the start the width is 2 s, the height is 0.5, the first zero is π=3.14\pi=3.14 rad/s and the product reads 6.283, which is 2π2\pi. The pulse narrows and grows taller, and its area stays 1. At a width of 0.5 s the height is 2 and the first zero is 4π=12.574\pi=12.57 rad/s: four times narrower, four times wider in frequency, and still 1 at the centre, the area. At the end the width is 0.1250.125 s, the height is 8 and the first zero is 16π=50.2716\pi=50.27 rad/s. Squeezed further, the pulse heads toward δ(t)\delta(t), whose spectrum is flat at 1: every frequency, equally.

The pulse has not yet become δ(t)\delta(t) at the end: there X(j20)=0.759X(j20)=0.759, still below 1. The unit-area pulse that Impulse, step and ramp (3.1) shrank towards δ(t)\delta(t) is this one, and as W→0W\to0 the spectrum becomes flat at 1.

A click is the example to remember. It is so short that it contains every pitch. A long steady note lasts a long time and contains one.

A decaying exponential: magnitude and phase

The pulse was symmetric, so its sum stayed on the real axis. A struck bell is not: its sound starts at once and then decays. I model it with x(t)=e−tu(t)x(t)=e^{-t}u(t), which is 0 before t=0t=0 and e−te^{-t} after.

Wound at rate ω\omega, it becomes e−te−jωt=e−(1+jω)te^{-t}e^{-j\omega t}=e^{-(1+j\omega)t}, which is a shrinking spiral, as on Complex exponentials & phasors (3.4). With a=−(1+jω)a=-(1+j\omega) in ∫eat dt=eat/a\int e^{at}\,dt=e^{at}/a, and the spiral shrinking to 0,

X(jω)=∫0∞e−(1+jω)t dt=11+jω.X(j\omega)=\int_0^\infty e^{-(1+j\omega)t}\,dt=\frac1{1+j\omega}.

This is a complex number, so I read it by its size ∣X∣\lvert X\rvert and its angle ∠X\angle X. Dividing by a complex number divides the lengths and subtracts the angles, as on Fourier series and LTI systems (7.4). So ∣X∣=1/1+ω2\lvert X\rvert=1/\sqrt{1+\omega^2} and ∠X=−arctan⁡ω\angle X=-\arctan\omega.

The winding instrument appears again, now with e−te^{-t} for t≥0t\ge0, wound into the spiral e−(1+jω)te^{-(1+j\omega)t}. Watch the sum shrink and turn back as the rate rises from 0 to 10 rad/s.

Winding at any rate: a decaying exponential

e^(−t) for t ≥ 0, wound at a rate ω and added up.

No winding: the area under e^(−t) is 1.

winding rate ω
0.000 rad/s
size |X|
1.000
angle ∠X
0.0°
0.00 / 10.00 s
Describe this picture

A plane with the spiral for the current rate and the dot labelled “sum (signal × s)”. Two strips are drawn against ω from 0 to 10 rad/s: ”∣X∣\lvert X\rvert (signal × s)” and ”∠X\angle X (degrees)”. The readouts are “winding rate ω”, “size |X|” and “angle ∠X”. The rate rises from 0, holds at 1 rad/s after 3 s, and ends at 10 rad/s, where the readouts show 0.100 and −84.3°. There is no control.

With no winding, the spiral is a straight segment from 1 to 0 and the sum is 1, the area under e−te^{-t}. Winding faster, the spiral turns more tightly, and the sum shrinks and turns back. At 1 rad/s it is 0.707 long and 45° behind.

Those are the numbers 0.707∠−45°0.707\angle-45° of the RC circuit in 7.4, since 1/(1+j)1/(1+j) has length 1/21/\sqrt2 and angle −45°-45°. Why a circuit’s response is the transform of its own decay is the subject of the page Frequency response and Bode plots (8.4). At 10 rad/s the sum is smaller and turned nearly a quarter turn back: 0.0995∠−84.3°0.0995\angle-84.3°, which the readouts show as 0.100 and −84.3°.

The strips show only ω≥0\omega\ge0. For a real signal, the negative side is the mirror image: X(−jω)=X∗(jω)X(-j\omega)=X^*(j\omega), so the size is even and the angle is odd. Here X∗X^* is the conjugate, the mirror image of XX, from Complex numbers for signals (3.3).

Build it back from a band of frequencies

The inverse transform adds up arrows over all frequencies. Suppose a system keeps only the band ∣ω∣<ωc\lvert\omega\rvert<\omega_c and drops the rest, as a speaker that cannot reproduce high frequencies does to a sharp click. What comes back? Here ωc\omega_c is the edge of the kept band.

For the unit pulse, the rebuilt signal is 12π∫−ωcωcX(jω)ejωt dω\tfrac1{2\pi}\int_{-\omega_c}^{\omega_c}X(j\omega)e^{j\omega t}\,d\omega. It comes back rounded, with a bump beside each edge of the pulse. A wider band narrows the bump towards the edge, but the top of the bump heads for 1.091.09 and not for 1. That is about 9 % of the jump from 0 to 1, the same bump as on Convergence and the Gibbs phenomenon (7.3).

The band widens from ωc=4π\omega_c=4\pi to 32π32\pi rad/s in the next instrument. Watch the bump beside each edge of the rebuilt pulse, and the tallest point, in 7.3’s meaning: the highest point of the rebuilt curve.

Width and band: rebuild from a band

The unit pulse rebuilt from a band of frequencies only.

Frequencies up to 4π rad/s: a rounded pulse whose top wobbles, highest at ±0.25 s.

band edge
12.566 rad/s
tallest point
1.123 at ±0.250 s
value at the edge t = 0.5
0.475
0.00 / 12.00 s
Describe this picture

The upper panel shows a dashed “target” and the “rebuilt” curve, with rings at the “tallest point” and a square marker at the “edge” t=0.5t=0.5. The lower panel is the pulse spectrum from −112-112 to 112112 rad/s, with the “kept band” shaded and its edges marked “−ω_c” and “ω_c”. The readouts are “band edge”, “tallest point” and “value at the edge t = 0.5”. The band widens from 4π4\pi to 32π32\pi rad/s, holding at three frames: 4π4\pi, 16π16\pi and 32π32\pi.

With frequencies up to 4π4\pi rad/s, 12.566 rad/s, the rebuilt pulse is rounded and its top wobbles. The tallest point is 1.1231.123 at ±0.250\pm0.250 s and the value at the edge is 0.4750.475. As the band widens, more frequencies are added back, and the bump moves toward the edge.

At 16π16\pi rad/s the tallest point is 1.0961.096 at ±0.438\pm0.438 s and the edge value is 0.4940.494: the bump has moved to the edge and narrowed, and its top barely fell. At 32π32\pi rad/s the tallest point is 1.0931.093 at ±0.469\pm0.469 s and the edge value is 0.4970.497.

The top heads for 1.09, about 9 % of the jump from 0 to 1, as in 7.3. At the edge itself, the curve passes through the middle, 0.5. The three held frames sit on high points. Between them the tallest point is not steady: it wobbles between about 1.06 and 1.12 as the band widens, while its position moves towards the edge, and it settles towards 1.09. It stays well above 1 however wide the band, and the edge value approaches 0.50.5.

The maths behind it · change of basis

Describing a signal by “how much of each spinning arrow it contains” instead of “its value at each instant” is a re-expression of the same signal in different building blocks. Linear algebra calls that a change of basis. For sampled signals it is a matrix (13.5); with more and more rows it becomes the integral of this page.

The maths behind it · characteristic functions

Wind a probability density, a curve whose area is 1 and which says how likely each value is, as this page winds a pulse. The sum is what statisticians call its characteristic function. “Lines get shorter as they crowd, while the curve stays put” is the step from the probabilities of separate values to a density.

Worked example

  1. Unit pulse. X(jω)=∫−1/21/2e−jωt dt=ejω/2−e−jω/2jω=2sin⁡(ω/2)ω=sin⁡(ω/2)ω/2X(j\omega)=\displaystyle\int_{-1/2}^{1/2}e^{-j\omega t}\,dt=\frac{e^{j\omega/2}-e^{-j\omega/2}}{j\omega}=\frac{2\sin(\omega/2)}{\omega}=\frac{\sin(\omega/2)}{\omega/2}. Then X(0)=1X(0)=1, X(jπ)=0.6366X(j\pi)=0.6366, X(j2π)=0X(j2\pi)=0 and X(j3π)=−0.2122X(j3\pi)=-0.2122.
  2. Lines and curve. Unit pulses every TT s have ck=1TX(jkω0)c_k=\tfrac1TX(jk\omega_0). For T=2T=2 (ω0=π\omega_0=\pi), ck=0.5, 0.3183, 0, −0.1061c_k=0.5,\ 0.3183,\ 0,\ -0.1061 for k=0k=0 to 3, and T ck=1, 0.6366, 0, −0.2122T\,c_k=1,\ 0.6366,\ 0,\ -0.2122. For T=4T=4, T ck=1T\,c_k=1, 0.90030.9003, 0.63660.6366, 0.30010.3001, 00, −0.1801-0.1801 for k=0k=0 to 5. For T=8T=8, ck=0.1250c_k=0.1250, 0.12180.1218, 0.11250.1125, 0.09800.0980, 0.07960.0796 for k=0k=0 to 4.
  3. Density. The band from 3.1 to 3.2 rad/s carries about X(jπ) Δω/2π=0.637×0.1/6.283=0.0101X(j\pi)\,\Delta\omega/2\pi=0.637\times0.1/6.283=0.0101. The mirror band carries the same. At exactly one frequency the band is zero wide and carries nothing.
  4. Unit-area pulse of width WW. X(jω)=sin⁡(ωW/2)ωW/2X(j\omega)=\dfrac{\sin(\omega W/2)}{\omega W/2}, with first zero 2π/W2\pi/W, so width times first zero is 2π2\pi. For W=0.125W=0.125 s the first zero is 50.2750.27 rad/s and X(j20)=sin⁡(1.25)/1.25=0.7592X(j20)=\sin(1.25)/1.25=0.7592.
  5. Exponential, a=1a=1. ∫0∞e−(1+jω)t dt=11+jω\displaystyle\int_0^\infty e^{-(1+j\omega)t}\,dt=\frac1{1+j\omega}. At ω=1\omega=1: ∣1+j∣=2\lvert1+j\rvert=\sqrt2, so 0.7071∠−45.00°0.7071\angle-45.00°. At ω=2\omega=2: 0.4472∠−63.43°0.4472\angle-63.43°. At ω=5\omega=5: 0.1961∠−78.69°0.1961\angle-78.69°. At ω=10\omega=10: 0.0995∠−84.29°0.0995\angle-84.29°.
  6. Band-limited pulse. Keeping only ∣ω∣<ωc\lvert\omega\rvert<\omega_c, the tallest point of the rebuilt unit pulse is 1.12261.1226 at ωc=4π\omega_c=4\pi, 1.10391.1039 at 8π8\pi, 1.09621.0962 at 16π16\pi and 1.09281.0928 at 32π32\pi. The limit is 1.08951.0895, about 9 % above the top of the pulse.

Where you’ll meet this

A spectrum analyser on a single sound, a click or a drum hit, shows a curve and not a row of lines, because the sound does not repeat. The trade of step 4 is why a short click is spread over many frequencies, and why a high-quality loudspeaker needs a wide band to reproduce one cleanly. The transform exists, in the sense of this page, when the area under ∣x∣\lvert x\rvert is finite, which a pulse and a decaying exponential satisfy. A signal that never dies out, such as a steady tone, needs spikes, and that is the subject of the page Transforms of common signals (8.3).

Each operation on a signal has a matching change in its spectrum. A delay turns the angles, a squeeze stretches the curve, and these rules are the page Properties of the Fourier transform (8.2). The same limit, applied to sampled data, gives The DTFT (12.2). Band-limiting and the rebuild of a signal from its samples return in The sampling theorem (10.2) and Reconstruction (10.3).

Reference card

QuantityFormulaNotes
Fourier transformX(jω)=∫−∞∞x(t)e−jωtdtX(j\omega)=\displaystyle\int_{-\infty}^{\infty}x(t)e^{-j\omega t}dtunits signal × s; Hz form X(f)=∫x e−j2πftdtX(f)=\int x\,e^{-j2\pi ft}dt, ω=2πf\omega=2\pi f
Inversex(t)=12π∫−∞∞X(jω)ejωtdωx(t)=\dfrac1{2\pi}\displaystyle\int_{-\infty}^{\infty}X(j\omega)e^{j\omega t}d\omegaadds up arrows over all frequencies
Densitythe band ω\omega to ω+Δω\omega+\Delta\omega carries about X(jω) Δω/2πX(j\omega)\,\Delta\omega/2\pione frequency alone carries nothing
Series from transformck=1TXT(jkω0)c_k=\dfrac1TX_T(jk\omega_0)XTX_T: transform of one period
Unit pulserect(t)↔sin⁡(ω/2)ω/2=sinc ⁣(ω2π)\mathrm{rect}(t)\leftrightarrow\dfrac{\sin(\omega/2)}{\omega/2}=\mathrm{sinc}\!\left(\dfrac{\omega}{2\pi}\right)sinc(x)=sin⁡πxπx\mathrm{sinc}(x)=\dfrac{\sin\pi x}{\pi x}; Hz form rect(t)↔sinc(f)\mathrm{rect}(t)\leftrightarrow\mathrm{sinc}(f); zeros at ±2π,±4π,…\pm2\pi,\pm4\pi,\dots
Unit-area pulse, width WW1Wrect(t/W)↔sin⁡(ωW/2)ωW/2\tfrac1W\mathrm{rect}(t/W)\leftrightarrow\dfrac{\sin(\omega W/2)}{\omega W/2}width × first zero =2π=2\pi; W→0W\to0: δ(t)↔1\delta(t)\leftrightarrow1
One-sided exponentiale−atu(t)↔1a+jωe^{-at}u(t)\leftrightarrow\dfrac1{a+j\omega}, a>0a>0∣X∣=1/a2+ω2\lvert X\rvert=1/\sqrt{a^2+\omega^2}, ∠X=−arctan⁡(ω/a)\angle X=-\arctan(\omega/a)
Real signalX(−jω)=X∗(jω)X(-j\omega)=X^*(j\omega)even magnitude, odd phase
Band-limited rebuildkeep ∣ω∣<ωc\lvert\omega\rvert<\omega_ctallest point → 1.09 beside each edge of a 0-to-1 pulse (about 9 % of the jump)
Existence∫∣x∣ dt<∞\int\lvert x\rvert\,dt<\infty is enoughsignals that never die out: 8.3

End of lesson 8.1

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