1. THE HUMAN EYE AND THE COLOURFUL WORLD
The Parts and their Functions of a Human Eye
Power of Accommodation and LDDV
Defects of Vision and their Correction -
Myopia, Hypermetropia and Presbyopia
Refraction through a Prism
Expression for Refractive Index of Prism
Dispersion
Rainbow
Atmospheric Refraction – Tyndall Effect, Apparent position & Twinkling of Stars, Delayed Sunrise & Sunset
Scattering of Light - Blue Colour of the Sky and Red Colour of the Sun
made by:- Akash patel school:- KV old cantt allahabad, INDIA
Medical ppt

2. THE HUMAN EYE

3. Cross Section through a Human Eye
Aqueous humour
Pupil

4. Parts and functions of a Human Eye
The human eye is like a camera.
Its lens forms an image on a light-sensitive screen called the retina.
Light enters the eye through a thin membrane called the cornea.
Cornea forms the transparent bulge on the front surface of the eyeball.
The eyeball is approximately spherical in shape with a diameter of about
2.3 cm.
Most of the refraction of light rays entering the eye occurs at the outer
surface of the cornea.
The crystalline lens merely provides the finer adjustment of focal length
required to focus objects at different distances on the retina.
Iris is a dark muscular diaphragm behind the cornea and it controls the
size of the pupil.
The pupil regulates and controls the amount of light entering the eye.
The eye lens forms an inverted real image of the object on the retina.

5. The eye lens is composed of a fibrous, jelly-like material.
Its curvature can be modified to some extent by the ciliary muscles.
The change in curvature can thus change the focal length of the lens.
The retina is a delicate membrane having enormous number of light-
sensitive cells.
The light-sensitive cells get activated upon illumination and generate
electric signals.
These signals are sent to brain via optic nerves.
The brain intercepts these signals and finally processes the information
for our perception.

6. Power of Accommodation
The ability of the eye lens to adjust its focal length is called accommodation.
The eye lens is composed of a fibrous, jelly-like material and its curvature can be modified by the ciliary muscles. Hence, the focal length can be changed as per the requirement.
When the muscles are relaxed, the lens becomes thin. The radius of curvature and hence the focal length increases. This enables us to see the distant objects clearly.
When we look at the objects closer to they, ciliary muscles contract decreasing the radius of curvature and hence the focal length. This enables us to see the nearby objects clearly.
Least Distance of Distinct Vision (LDDV):
The minimum distance, at which objects can be seen most distinctly without strain, is called Least Distance of Distinct Vision(LDDV). For a normal eye, LDDV is 25 cm.

7. DEFECTS OF VISION AND THEIR CORRECTION

8. Myopia or Short-sightedness or Near-sightedness
A person with myopic eye can see nearby objects clearly but cannot see distant objects distinctly.
Such a person may clearly see upto a distance of a few metres.
In myopic eye, the image of a distant object is formed in front of the retina and not on the retinal itself.
This defect may arise due to
excessive curvature of the eye lens (short focal length of the eye lens) or
(ii) Elongation of the eyeball.
Myopia can be corrected by using a concave lens of suitable power(focal length).

9. Myopic Eye corrected with Concave Lens
Normal Eye O I
Near Point
LDDV = 25 cm
Myopic Eye O I
LDDV = 25 cm O I
LDDV = 25 cm O
LDDV = 25 cm I O I I
LDDV = 25 cm
Myopic Eye corrected with Concave Lens

10. Hypermetropia or Long-sightedness or Far-sightedness
A person with hypermetropia can see distant objects clearly but cannot see nearby objects distinctly.
Such a person may has to keep a reading material much beyond 25 cm from the eye for comfortable reading.
In hypermetropic eye, the image of a nearby object is formed behind the retina and not on the retinal itself.
This defect may arise due to
(i) long focal length of the eye lens or
(ii) Very small size of the eyeball.
Hypermetropia can be corrected by using a convex lens of suitable power (focal length).

11. Hypermetropic Eye corrected with Convex Lens
Normal Eye O I
Near Point
LDDV = 25 cm
Hypermetropic Eye O I
LDDV = 25 cm O I
LDDV = 25 cm
LDDV = 25 cm I O O I I
LDDV = 25 cm
Hypermetropic Eye corrected with Convex Lens

12. Presbyopia
The power of accommodation of the eye usually decreases with ageing.
People can not see nearby objects comfortably and distinctly without corrective eye-glasses.
This defect is called presbyopia.
It arises due to
gradual weakening of the ciliary muscles and
diminishing flexibility of the eye lens.
Sometimes, a person may suffer from both myopia and hypermetropia. Such
people require bi-focal lenses which consists of both concave and convex
lenses. The upper portion is concave for distant vision and the lower portion
is convex for near vision.

13. REFRACTION OF LIGHT THROUGH A TRIANGULAR PRISM - Activity
Refracting Surfaces A
Prism
Eye S P R Q e i N2 N1

14. Refraction of Light through Prism:B C N1 N2 D δ e i Q R r1 O r2 S P μ
Prism
Refracting Surfaces
i + e = A + δ

15. DISPERSION OF WHITE LIGHT THROUGH A PRISM
The phenomenon of splitting a ray of white light into its constituent colours (wavelengths) is called dispersion and the band of colours from violet to red is called spectrum (VIBGYOR). A δr D N δv
ROYGB I V
White light B C
Screen

16. Recombination of spectrum of white light:

17. RAINBOW
A rainbow is a natural spectrum which is caused by dispersion of sunlight by tiny water droplets present in the atmosphere after a rain shower.
The incident sunlight with suitable angle of incidence is refracted, dispersed, internally reflected and finally refracted out by the rain drops.
Due to the dispersion and internal reflection, different colours reach the eye of the observer.
A rainbow is always formed in a direction opposite to that of the Sun.

18. Formation of Rainbow Rain drop Sunlight 43º 41º
A line parallel to Sun’s ray
Eye

19. RAINBOW

20. ATMOSPHERIC REFRACTION
Refraction of light by earth’s atmosphere is called atmospheric refraction.
Flickering of objects above a fire:
The apparent random wavering or flickering of objects can be seen through a turbulent stream of hot air rising above a fire.
The air just above the fire becomes hotter than the further up. The hotter air is lighter than the cooler air above it, and has a refractive index slightly less than that of the cooler air.
Since the physical conditions of the refracting medium (air) are not stationary, the apparent position of the object, as seen through the hot air, fluctuates. This wavering is therefore due to an effect of atmospheric refraction on a small scale in the local environment.

21. Twinkling of Stars:
The twinkling of a star is due to atmospheric refraction of starlight.
The atmospheric refraction occurs in a medium of gradually changing refractive index.
Since the atmosphere bends starlight towards the normal, the apparent position of the star is slightly different from its actual position.
The star appears slightly higher (above) than its actual position when viewed near the horizon.
This apparent position is not stationary, but keeps on changing slightly, since the physical conditions of the earth’s atmosphere are not stationary.
Since the stars are very distant, they approximate point-sized sources of light.
As the path of rays of light coming from the star goes on varying slightly, the apparent position of the star fluctuates and the amount of light entering the eye flickers- the star sometimes appear brighter, and at some other time, fainter which gives the twinkling effect.
Real position of the Star
Apparent position of the Star
Density of Atmosphere & Refractive index increase
Eye

22. Why Planets do not twinkle?
The planets are much closer to the earth, and are thus seen as extended sources.
Since it is the collection of large number of point-sized sources of light, the total variation in the amount of light entering into the eye from all the individual sources will average out to zero, thereby nullifying the twinkling effect.
Advance Sunrise and Delayed Sunset:
The Sun is visible to us about 2 minutes before the actual sunrise, and about minutes after the actual sunset because of atmospheric refraction.
Apparent position of the Sun
Atmosphere
Horizon
Earth
Real position of the Sun

23. SCATTERING OF LIGHT Tyndall Effect:
The earth’s atmosphere is a heterogeneous mixture of minute particles. These particles include smoke, tiny water droplets, suspended particles of dust and molecules of air.
When a beam of light strikes such fine particles, the path of the beam becomes visible.
The light reaches us, after being reflected diffusedly by these particles.
The phenomenon of scattering of light by the colloidal particles gives rise to Tyndall Effect.
Tyndall Effect can be seen when a fine beam of sunlight enters a smoke-filled room through a small hole. In this, scattering of light makes the particles visible.
It can also be seen when sunlight passes through a canopy of a dense forest. In this, tiny water droplets in the mist scatter light.
The colour of the scattered light depends on the size of the scattering particles.
Very fine particles scatter mainly blue light while particles of larger size scatter light of longer wavelengths. If the size of the scattering particles is large enough, then, the scattered light may even appear white.

24. SCATTERING OF LIGHT - Activity
Conc. Sulphuric acid L1 L2
Screen S I
Sodium thio sulphate solution (hypo)

25. SCATTERING OF LIGHT BY TINY WATER DROPLETS IN THE MIST

26. SCATTERING OF LIGHT BY SMOKE & COLLOIDAL PARTICLES

27. Scattering of Light – Blue colour of the sky and Reddish appearance of the Sun at Sun-rise and Sun-set:
Less Blue colour is scattered
Earth
Horizon
Atmosphere
Other colours mostly scattered

28. The molecules of the atmosphere and other particles that are smaller than the longest wavelength of visible light are more effective in scattering light of shorter wavelengths than light of longer wavelengths. The amount of scattering is inversely proportional to the fourth power of the wavelength. (Rayleigh Effect)
Light from the Sun near the horizon passes through a greater distance in the Earth’s atmosphere than does the light received when the Sun is overhead. The correspondingly greater scattering of short wavelengths accounts for the reddish appearance of the Sun at rising and at setting.
When looking at the sky in a direction away from the Sun, we receive scattered sunlight in which short wavelengths predominate giving the sky its characteristic bluish colour.

29. THE END
Medical ppt