In recent years there have
been enormous advantages in the application of CCD technology. The charge coupled
device, or CCD, is a means of capturing an image electronically. As developments have
progressed and the number of CCD cameras ha increased the price has fallen and it is now
possible to buy a CCD camera quite cheaply.
The optical parts of a CCD camera
are similar to those of one using 'conventional' film. It is the method of detecting and storing
the image that is different.
With a conventional film the image of the object is
focused on a light sensitive surface and as light falls on the film a chemical change takes
place. The resolution of fine detail depends on the size of the 'grains' of chemical on the film,
typical grain having a diameter of around 10-6 m.
The imaging area, or chip, in the
CCD is composed of 'cells' made of thin layers silicon. As light falls on its surface electron-
hole pairs are formed and a charge is built up. The charge depends on the total energy of
the light that falls on the cell during the exposure. Therefore the longer the exposure and the
brighter the light the more charge is built up on the individual cell. The cells are scanned
electronically and a digital version of the image is built up. This can be downloaded to a
computer for processing by the appropriate software.
The imaging area of a CCD
camera consists of a grid of a large number of these cells or pixels. Cameras with 2 million
pixels on the chip are extensively used although 4 million is now becoming the accepted
standard. The chip is typically about 10 mm x 5 mm and so each pixel has an area of
roughly 2.5x10-5 mm. In my CCD camera that I use with my telescope the chip has 752x852
pixels in a 6.5x4.8 mm active area.
Three examples of the kind of images
obtained with this camera can be seen in Figure 1.