Array of p-doped Si pixels + Convert incident photons to electronic charge What is a CCD? ➲ Astronomical ➲ Space and Earth Observation ➲ Life Sciences ➲ Fast lifetime fluorescing ➲ Scientific ➲ X-Ray spectroscopy ➲ Health Care ➲ Dental X-Rays ➲ Ophthalmology CCD231-84 Hubble Telescope
+ Semiconductor Physics + Two types of doped semiconductors: + P-type (excess holes) + N-type (excess electrons) + Photon incident to CCD + Excitation of electron across energy band-gap + Creation of an exciton (electron- hole pair) at semiconductor interface
through gates + n-channel formed beneath gates + Excitons formed in n-channel + Electrons and holes separated by electric field + Holes to substrate + Electrons to surface + Formation of depletion region Device operation +V V V n-Channel
+V +V V V + Positive voltage bias through gates + n-channel formed beneath gates + Excitons formed in n-channel + Electrons and holes separated by electric field + Holes to substrate + Electrons to surface + Formation of depletion region + Charge in wells moved along row alternating voltage on gates + Moved to IC to be manipulated
flux. + Quantum Efficiency + Spectral Response + Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise Number of photons converted to charge in the pixel.
+ Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise Wavelength (nm) Quantum Efficiency (%) Range of wavelengths absorbed by the CCD and QE obtained. Change of coating will change the spectral response.
+ Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise Output Current Photo- generation pairs Depletion Region pairs Surface pairs Neutral Bulk pairs Sources of additional Charge “noise” Reduced through cooling
from the CCD array Effective frame-rate of the camera + Quantum Efficiency + Spectral Response + Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise
+ Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise Measure of the transfer characteristic of the CCD output.
+ Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise Maximum signal which can be stored, transferred and read from a pixel in the CCD. Can be determined through saturation of the pixel well, or other specified limit
+ Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise Measure of ability to determine maximal difference between dark/light limits. Ratio of maximum possible signal (full well) vs. the total noise signal (in the dark)
+ Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise Range of wavelengths of photons that can be converted to charge. Areas of application for the CCD
+ Dark Current + Maximum Readout Freq + Output Responsivity + Peak Signal + Dynamic Range + Spectral Range + Readout Noise A measure of the additional charge “noise” (Dark Current) added to the output frame. Removed through ‘Dark Frame’ subtraction and additional cooling.
Nitrogen + Peltier based coolers + CCD coating to change spectral response/QE + Readout frequency can be increased through the use of on chip charge storage + Increased Resolution + QE increased through Back- Illumination fabrication Other e2v Imaging Systems: • CMOS • L3VISION