Catania Astrophysical Observatory Laboratory for Detectors
Charge Coupled Device (CCD)
Physical description of a CCD
CCD main functions
By schematizing, four fundamental moments can be identified:
- charge generation by photoelectric effect;
- charge collection through potential well generation;
- charge transfer, by varying the electrode potentials appropriately;
- charge extraction by meansof the output circuit.
Typical sructure of a three phase CCD
The figure on the right shows the scheme of a three phase CCD. In this case the pixel is made by 3 MOS elements. Along the vertical columns the separation is obtained with the stop channels (dashed lines).
In this scheme 4 fundamental areas can be identified:
- The image area, sensitive to radiation and in which charges accumulate.
- The storage area, cwhich is covered so as not to be sensitive to radiation, in which the charges generated in the image area are moved to allow a reading free from further radiation contamination (in practice the use of the shutter is eliminated).
- The read-ou register, where an entire row of pixels is transferred, and where the transfer of each pixel to the output circuit begins. Also in this register the pixel is made with 3 MOS elements.
- The output circuit that allows the charge extraction.
Lessons on CCDs and other photon detectors are available in PDF (Italian language)
Characteristics of some CCDs used in astronomical instruments
e2v 02-06 | Series | |
e2v 15-11 | Series | |
e2v 05-20 | Series | |
e2v 05-30 | Series | |
e2v 42-80 | (Mounted in a mosaic of 2 x 1on the focal plane of OIG and SARG instruments of the TNG) | |
LORAL 2K3eb | (Back ill. 2048X2048 pixels S. N. W1-1) | |
LORAL 2K3eb | (S. N. W1-1(0,0). Used on the DOLORES spectrograph of the TNG) |