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OXP-19 Camera

  Topics:
Pinhole Camera
Objective
CCD Sensor
Magnification
Depth of Field
 

Giovanni Antonio Canaletto
1697 – 1768

 


The principle of creating an image through projection on a surface is known since ancient times. Aristotle observed images of the sun through holes generated by the leaves of a tree, while Arab scientists used this principle in astronomy to observe the solar eclipses. The most clear and detailed description is made by Leonardo da Vinci in his work “Codice Atlantico” where for the first time, the structure of the human eye is commented as a “camera obscura”.
But most of our respect should be paid to Giovanni Antonio Canaletto. As a painter he used the principle of the camera obscura in a very practical and commercial application. Although he did not take photographs as one understands it today, he imaged scenes and objects on canvas through a narrow hole in a curtain and painted them. With the help of this technique he was able to produce more than 900 paintings during his period. Later Giovanni Battista Della Porta suggested for the first time that a lens may be applied to the hole. This was the initial step for the invention of the portable “camera obscura” as a working tool for outlining at that time.
In the frame of this experiment a camera obscura is built through combining a narrow diaphragm and a CCD array. Parameters like diaphragm size, position and the influence of lenses on the brightness, sharpness and dimensions of the image are investigated. Camera objectives can be simulated by sets of lenses and a variable diaphragm demonstrates the effect of screening.




 

Examples of Investigation and Measurement


Model of camera obscura
A pinhole camera is set up, consisting of a narrow diaphragm and – instead of the classical matt screen – a CCD array connected to a monitor. In this arrangement even dim images are detected and do not need to be observed in a dark room.

Influence of diaphragm size and position
By increasing the size of the diaphragm the brightness increases, but the sharpness of the image becomes worse. By changing the distance between diaphragm and CCD array the magnification of the pinhole camera is varied.

Influence of optics
The use of collimating lenses in front and behind the diaphragm increases the brightness and improves the sharpness dramatically. Several types of objectives can be set up and investigated. A variable diaphragm demonstrates the effect of screening and the changes of the depth of field are observed.

 


 

 

 

 

OXP-19   Required Equipment


1  
 


02.0300
 

 


Profile rail OCM 650, 300 mm

The high precision optical rails are made out of special anodized aluminum. The rails are the base for various modules attached to carriers.
 




 

1

02.1024

Carrier OCM 650, 20 mm with attached plate holder

Using a spring loaded blade 50 x 50 mm, plates like filters or gratings can be fixed onto this module. The carrier allows the direct attachment to the optical rail. The carrier 20 mm and the holder are made out of special anodized aluminum.
 

2
2

02.2126
02.2132

Mounting plate OCM 650 for click 25, including carrier 20 mm
Mounting plate OCM 650 for click 30, including carrier 20 mm

Mounting plates are used to hold optical mounts. A characteristic feature of the mounting plates is the “click” mechanism of the inserts based on spring loaded spheres. Snapping in the groove of the inserted click mount, the optical element is kept in an exact position. On the other hand, the system allows a quick and easy change of the mounted inserts.
The mounting plates are made out of special anodized aluminum. Mounted onto the carrier 20 mm, the mounting plates can be placed onto an optical rail.
 

1 02.2528

Click mount 25 mm with 0,5 mm hole aperture

This click mount 25 mm contains a disk with a 0.5 mm hole aperture and is commonly used to reduce the acceptance angle of a photodetector. The click mount can be fixed onto a mounting plate (02.2126).

1 02.2529

Click mount 25 mm with 0,1 mm hole aperture

This click mount 25 mm contains a disk with a 1 mm hole aperture and is commonly used to reduce the acceptance angle of a photodetector. The click mount can be fixed onto a mounting plate (02.2126).

1
1
1
1
04.0051
04.0053
04.0060
04.0062

Biconvex lens f=100 mm, mounted in click 30 mount
Biconvex lens f=150 mm, mounted in click 30 mount
Plano convex
lens f=40 mm, mounted in click 30 mount
Plano convex lens f=60 mm, mounted in click 30 mount

different glass lenses are mounted onto a special anodized aluminum click mount 30 mm by two threaded mounting rings to be used in connection with a mounting plate (02.2132).
 

1 04.0138

IR block filter, size 50x50x3

This glass filter is used for suppressing IR light coming from a light source. The filter can be fixed onto a plate holder (02.1024).
Dim:
50 mm x 50 mm x 3 mm
 

 

1 04.0308

Iris aperture mounted in click 25 mount, max. opening 14 mm

The continuously adjustable laminar aperture limits the diameter of the beam from 1 mm to a maximum of 14 mm. The iris aperture is mounted onto a special anodized aluminum click mount 25 mm by a threaded mounting ring to be used in connection with a mounting plate (02.2126).
 

1 09.2930

CCD array with monitor

The colour CCD array is fixed in a sleeve mountable onto a click 25 mounting plate 02.2126. It has a power supply and can be connected to 230 VAC / 50 Hz directly. The CCD can be connected to the monitor via a BNC cable. The CRT colour monitor screen has a diameter of 300 mm and is equipped with a BNC input.

Further specifications of the camera:
Video System: NTSC / PAL
Effective pixels: 628 x 582
S/N ratio: more than 48 dB
Sync frequency: NTSC 60 Hz / PAL 50 Hz.

 







 


 


 




 

 

Experiments

OXP-01 Refraction of Light

OXP-02 Prisms

OXP-03 Lenses

OXP-04 Reflection & Transmission

OXP-05 Beam Bending

OXP-06 Refractometer

OXP-07 Diffraction of Light

OXP-08 Optical Gratings

OXP-09 Spectral Analysis

OXP-10 Interference

OXP-11 Interferometer

OXP-12 Holography

OXP-13 Polarisation

OXP-14 Double Refraction

OXP-15 Colour Mixing

OXP-16 Optical Filters

OXP-17 Absorption & Emission

OXP-18 Image Projection

OXP-19 Camera

OXP-20 LED & Laser Diode

 

Kits

Basic Kit

Complete Kit

Advanced Kit