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Team:
Dinh Cong Huy
Nguyen Thai Long
Bui Viet Hung
Nguyen Duc Nam
HUT- 17/10/2008
Gratings and application
Mechatronics Engineering- Advanced Training Program

Grating: a system of multi close equidistant and
parallel lines or bars, especially lines ruled on a
polished surface, used for producing spectra by
diffraction called also diffraction grating.

Diffraction grating: is an optical device used to learn
the different wavelength or color contained in a
beam of light. The device usually consist of thousand
of narrow, closely spaced parallel slits (or grooves).
Figure 1:
- Diffraction grating: is an
optical device used to learn
the different wavelength or
color contained in a beam of light.
The device usually consist of thousands of
narrow, closely spaced parallel slits (or grooves).
- Used for producing spectra.(Fig 1)
I- INTRODUCTION
Fig 2: The first
diffraction
grating was
made by


Fraunhofer
(which is called
Fraunhofer
diffraction).
II- Background of topic

1. Single – slit diffraction.

2. Double- slits diffraction.

3. Multi- slits diffraction.

4. Diffraction gratings.

5. Quiz.
II- Background
The smaller the slit, the broader the
entire the diffraction pattern.
1. Single slit diracon:
Phenomena: the beam spreads out
vercally aer passing through the slit.
Denote:
a- the width of the slit
d- the distance between slit and
screen
θ - the angle between the
perpendicular to the slit a line
from the center of the slit to a
point P on the screen
Condition for dark fringe:

sin m
a
λ
θ
=
m= 1,2,3…
m
m
y d
a
λ
=
2
sina
π
β θ
λ
=
( )
( )
2
2
0 0
sin sin /
sin( / 2)
/ 2 sin /
a
I I I
a
π θ λ

β
β π θ λ
 
 
 
 
 
= =
 
 
 
 
 
Posion of the mth dark fringe:
The phase di'erence
between the phase of
light of the upper and
lower trip:
The intensity :
2.Double slits diffraction:
Diffraction
envelope
Inference fringe
- must consider not only diffraction due to the individual slits but also the
interference of wave coming form different source.
-intensity:
2
2
0
sin( / 2)

cos
2 / 2
I I
φ β
β
 
=
 
 
2
sin
d
π
φ θ
λ
=
Where: is the phase
di'erence at point P of 2
incident lights, and is
calculated by the
formula:
φ
2
sina
π
β θ
λ
=
And : is the phase
di'erence of wave at P

from the top trip with
respect to the wave
received from the
bo*om trip:
β
3.Multiple slits diffraction:
-
Constructive interference occurs for rays
at angle θ satisfy: d.sinθ=mλ
(m= 0,±1,±2,±3…)
- The maxima are the same position as
for two slits diffraction with the same
spacing d.
Q: Why occurs such this
coincidence ?
Interference patterns for N equally spaced very narrow slits.
 The greater the value of N, the narrower the principle maxima
become and the smaller the intensity of secondary maxima is.
4.Diffraction grating:
-
Thousands of very narrow and close slits.
-
The phenomena seen on the screen is similar to multi slits
diffraction.
-
Positions of the maxima are given by: d.sinθ= mλ
(m = 0,±1,±2, )
m=±1: first order lines
m=±2: second order lines


5. Quiz:

1. The pattern of double diffraction.

2. The pattern of interference.
Q:What is the difference?
A: No fundamental distinsion
III- APPLICATION OF DIFFRACTION

For instrument analytical chemistry.

In laser system

In astronomical application

In synchrotron radiation beam lines

Some special uses for grating : gratings as filters, gratings in fiber-
optic telecommunication, gratings as beam splitters, gratings as
optical couplers….

Resolving power, scattering and stray.
1. Resolving power:

Disperse a spectrum into its
wavelength components.

2 wavelengths:
The resolving power:
Where:

And:
1 2
λ λ

1 2
2
λ λ
λ
+
=
2 1
λ λ λ
∆ = −
N: the number slits of Diffraction
grating, m-th order diffraction.
R= N.m
R =
2. Spectrograph
Structure of a slit spectrograph
Sunlight spectrum

The important of this technique is to
astronomy.For example,to measure
sunlight spectrum.

With sunlight, people obtain
spectrum produced by a diffraction
grating has dark absorption lines.

The resolution of grating

spectrograph:

The greater the number of slits
N,the better the resolution;also,the
higher the order m of the diffration-
pattern maximum tthat we use,the
better the resolution.
.R N m
λ
λ
= =

3. Spectrometer:
Explanation about spectometer:

The light to be analyzed passes through a slit, and a collimated beam
of light is incident on the grating.

The diffracted light leaves the grating at angles that satisfy
Equation:

a telescope is used to view the image of the slit.

The wavelength can be determined by measuring the precise angles
at which the images of the slit appear for the various orders
sind m
θ λ
=
4. Some pictures in real life:


Rain-bow colors reflection and diffraction on the surface of
CD/DVD.

Fresnel mirror.
Dispersion through a prism.
Data soures:
1. University Physics with mordern physics 12
th

edition- Young
2.Fundamentals of Physics 7
th
edtion– Halliday,
Resnick, Walker.
3.
4.
Thanks for your attention!!!
Have a nice day!

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