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CCD ARCHITECTURES       267

                       benefit being about a 10-fold reduction in the number of thermoelectrons for every 20°C
                       decrease in temperature. Thermal noise can be reduced significantly by cooling the CCD
                       down to 	20°C or lower using a stack of 2–3 Peltier thermoelectric cooling devices. In
                       the presence of a current, a Peltier bimetallic strip becomes cold on one side and hot on
                       the other. The cold surface is mounted so that it is in indirect physical contact with the
                       CCD, while the heat on the other surface is removed by a fan or backed by a circulating
                       liquid cooling system. Astronomical cameras used for hour-long exposures are cooled
                       with liquid nitrogen. For biological specimens, acceptable images can be obtained from
                       exposures lasting just a few seconds or less from CCD cameras cooled to 0–10°C, but for
                       higher-quality, lower-noise images, deeper cooling to 	25°C to 	40°C is required. We
                       will deal with the noise components in a CCD image later in the chapter.



                       CCD ARCHITECTURES

                       CCD imagers come in three basic designs, which are shown in Figure 14-8 and
                       described as follows:

                        • Full-frame CCD. In this design, whose readout procedure was described in the pre-
                          ceding section, every pixel of the CCD surface contributes to the image. Exposures
                          are usually controlled by an electromechanical shutter, since the imaging surface
                          must be protected from incident light during readout of the CCD. Full-frame CCD
                          imagers are used for specimens requiring high dynamic range images and where the
                          time resolution can be on the order of a second or longer. The fastest frame rates in
                          so-called subarray mode are  10 frames/s and are limited by an electromechanical
                          shutter.
                        • Frame-transfer CCD. Cameras with frame-transfer CCDs are fast because expo-
                          sure and readout occur simultaneously. One-half of an elongated rectangular CCD
                          chip is masked at one end by an opaque cover (an aluminum coating on one-half of
                          the surface of the CCD), which is used as a storage buffer. After an exposure, all of
                          the pixels in the image half of the chip are transferred to pixels on the storage side
                          in 1 ms; the storage array is read out while the image array is being exposed for the
                          next picture. No camera shutter is needed because the time required for transfer
                          from the imaging area to the masked area ( 1 ms) is only a fraction of the time
                          needed for an exposure. A disadvantage is that only one-half of the potential imag-
                          ing surface of the chip can be used for imaging. Cameras of this type are chosen for
                          monitoring rapid kinetic processes such as in dye ratio imaging, where it is impor-
                          tant to maintain high spatial resolution and dynamic range.



                          Full frame             Frame transfer                Interline transfer

                                                                       Storage
                                                   Image   Storage
                                                                        Image


                       Figure 14-8
                       Types of CCD designs. (a) Full-frame CCD. (b) Frame-transfer CCD. (c) Interline-transfer
                       CCD.
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