KAE02150_16 [ONSEMI]

Interline CCD Image Sensor;
KAE02150_16
型号: KAE02150_16
厂家: ONSEMI    ONSEMI
描述:

Interline CCD Image Sensor

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KAE-02150  
1920 (H) x 1080 (V)  
Interline CCD Image Sensor  
The KAE−02150 Image Sensor is a 1080p (1920 × 1080) CCD in  
a 2/3optical format that provides exceptional imaging performance  
in extreme low light applications. Each of the sensor’s four outputs  
incorporate both a conventional horizontal CCD register and a high  
gain EMCCD register.  
www.onsemi.com  
An intra-scene switchable gain feature samples each charge packet  
on a pixel-by-pixel basis. This enables the camera system to determine  
whether the charge will be routed through the normal gain output or  
the EMCCD output based on a user selectable threshold. This feature  
enables imaging in extreme low light, even when bright objects are  
within a dark scene, allowing a single camera to capture quality  
images from sunlight to starlight.  
This image sensor is based on the 5.5-micron Interline Transfer  
CCD Platform, and features extended dynamic range, excellent  
imaging performance, and a flexible readout architecture that enables  
use of 1, 2, or 4 outputs. A vertical overflow drain structure suppresses  
image blooming, provides excellent MTF, and enables electronic  
shuttering for precise exposure control.  
Figure 1. KAE−02150 Interline CCD  
Image Sensor  
Table 1. GENERAL SPECIFICATIONS  
Parameter  
Architecture  
Typical Value  
Interline CCD; with EMCCD  
2004 (H) × 1144 (V)  
Features  
Total Number of Pixels  
Number of Effective Pixels  
Number of Active Pixels  
Pixel Size  
Intra-Scene Switchable Gain  
Wide Dynamic Range  
Low Noise Architecture  
Exceptional Low Light Imaging  
Global Shutter  
Excellent Image Uniformity and MTF  
Bayer Color Pattern and Monochrome  
1960 (H) × 1120 (V)  
1920 (H) × 1080 (V)  
5.5 mm (H) × 5.5 mm (V)  
Active Image Size  
10.56 mm (H) × 5.94 mm (V)  
12.1 mm (Diag.), 2/3Optical Format  
Aspect Ratio  
16:9  
Number of Outputs  
Charge Capacity  
Output Sensitivity  
1, 2, or 4  
20,000 e  
Applications  
44 mV/e  
Quantum Efficiency  
Mono/Color (RGB)  
Surveillance  
50% / 33%, 41%, 43%  
Scientific Imaging  
Medical Imaging  
Intelligent Transportation  
Read Noise (20 MHz)  
Normal Mode (1× Gain)  
Intra-Scene Mode (20× Gain)  
9 e rms  
< 1 e rms  
Dark Current (0°C)  
Photodiode, VCCD  
< 0.1 e /s, 6 e /s  
ORDERING INFORMATION  
See detailed ordering and shipping information on page 2 of  
this data sheet.  
Dynamic Range  
Normal Mode (1× Gain)  
Intra-Scene Mode (20× Gain)  
68 dB  
86 dB  
Charge Transfer Efficiency  
Blooming Suppression  
Smear  
0.999999  
> 1000 X  
−100 dB  
Image Lag  
< 1 e  
Maximum Pixel Clock Speed  
40 MHz  
Maximum Frame Rate  
Normal Mode, Intra-Scene Mode 60 fps (40 MHz), 30 fps (20 MHz)  
Package  
Cover Glass  
135 pin PGA  
Clear Glass, Taped  
NOTE: All Parameters are specified at T = 0°C unless otherwise noted.  
© Semiconductor Components Industries, LLC, 2016  
1
Publication Order Number:  
February, 2016 − Rev. 2  
KAE−02150/D  
KAE−02150  
ORDERING INFORMATION  
US export controls apply to all shipments of this product  
designated for destinations outside of the US and Canada,  
requiring ON Semiconductor to obtain an export license  
from the US Department of Commerce before image sensors  
or evaluation kits can be exported.  
Table 2. ORDERING INFORMATION  
Part Number  
Description  
Marking Code  
KAE−02150−ABB−JP−FA  
KAE−02150−ABB−JP−EE  
KAE−02150−FBB−JP−FA  
KAE−02150−FBB−JP−EE  
Monochrome, Microlens, PGA Package,  
Taped Clear Cover Glass (No Coatings), Standard Grade  
KAE−02150−ABB  
Serial Number  
Monochrome, Microlens, PGA Package,  
Taped Clear Cover Glass (No Coatings), Engineering Grade  
Color (Bayer RGB), Microlens, PGA Package,  
Taped Clear Cover Glass (No Coatings), Standard Grade  
KAE−02150−FBB  
Serial Number  
Color (Bayer RGB), Microlens, PGA Package,  
Taped Clear Cover Glass (No Coatings), Engineering Grade  
Table 3. EVALUATION SUPPORT  
Part Number  
Description  
KAE−02150−AB−A−GEVK  
KAE−02150 Evaluation Kit  
Lens Mount Kit for IT−CCD Evaluation Hardware  
LENS−MOUNT−KIT−C−GEVK  
See the ON Semiconductor Device Nomenclature document (TND310/D) for a full description of the naming convention  
used for image sensors. For reference documentation, including information on evaluation kits, please visit our web site at  
www.onsemi.com.  
www.onsemi.com  
2
KAE−02150  
DEVICE DESCRIPTION  
Architecture  
VOUT  
VOUT  
D3  
C3  
2072  
2072  
8
1
4
28  
1
10 24  
8
960  
960  
24 10  
1
28  
1
4
14  
8
1920 y 1080  
24 8  
8
24  
5.5 mm Pixels  
8
14  
4
1
4
1
28  
1
10 24  
8
960  
960  
8
24 10  
1
28  
2072 2070  
2070 2072  
VOUT  
VOUT  
B3  
A3  
Figure 2. Block Diagram  
Dark Reference Pixels  
electron-hole pairs within the individual silicon  
photodiodes. These photoelectrons are collected locally by  
the formation of potential wells at each photo-site. Below  
photodiode saturation, the number of photoelectrons  
collected at each pixel is linearly dependent upon light level  
and exposure time and non-linearly dependent on  
wavelength. When the photodiodes charge capacity is  
reached, excess electrons are discharged into the substrate to  
prevent blooming  
There are 14 dark reference rows at the top and bottom of  
the image sensor, as well as 24 dark reference columns on the  
left and right sides. However, the rows and columns at the  
very edges should not be included in acquiring a dark  
reference signal, since they may be subject to some light  
leakage.  
Active Buffer Pixels  
8 unshielded pixels adjacent to any leading or trailing dark  
reference regions are classified as active buffer pixels. These  
pixels are light sensitive but are not tested for defects and  
non-uniformities.  
ESD Protection  
Adherence to the power-up and power-down sequence is  
critical. Failure to follow the proper power-up and  
power-down sequences may cause damage to the sensor. See  
Power-Up and Power-Down Sequence section.  
Image Acquisition  
An electronic representation of an image is formed when  
incident photons falling on the sensor plane create  
www.onsemi.com  
3
KAE−02150  
Bayer Color Filter Pattern  
VOUT  
VOUT  
D3  
C3  
2072  
2072  
8
1
4
28  
1
10 24  
8
960  
960  
24 10  
1
28  
1
4
14  
8
1920 y 1080  
24 8  
8
24  
5.5 mm Pixels  
8
14  
4
1
4
1
28  
1
10 24  
8
960  
960  
8
24 10  
1
28  
2072 2070  
2070 2072  
VOUT  
VOUT  
B3  
A3  
Figure 3. Bayer Color Filter Pattern  
www.onsemi.com  
4
KAE−02150  
Physical Description  
Pin Grid Array and Pin Description  
H
G
F
E
D
C
B
A
17 16 15 14 13 12 11 10 9  
8 7 6 5 4 3 2 1  
Figure 4. PGA Package Designations (Bottom View)  
Table 4. PIN DESCRIPTION  
Pin  
A02  
A03  
A04  
A05  
A06  
A07  
A08  
A09  
A10  
A11  
A12  
A13  
A14  
A15  
A16  
A17  
B01  
B02  
B03  
Label  
V3B  
Description  
VCCD Bottom Phase 3  
N/C  
No Connection  
RG2a  
N/C  
Amplifier 2 Reset, Quadrant A  
No Connection  
VDD23ab  
H1BEMa  
H2Ba  
GND  
Amplifier 2 and 3 Supply, Quadrants A, B  
EMCCD Barrier Phase 1, Quadrant A  
HCCD Barrier Phase 2, Quadrant A  
Ground  
H2Bb  
H1BEMb  
VDD23ab  
N/C  
HCCD Barrier Phase 2, Quadrant B  
EMCCD barrier phase 1, Quadrant B  
Amplifier 2 and 3 Supply, Quadrants A, B  
No Connection  
RG2a  
N/C  
Amplifier 2 Reset, Quadrant B  
No Connection  
V3B  
VCCD Bottom Phase 3  
ESD  
ESD Protection Disable  
DEVID  
V4B  
Device ID Resistor  
VCCD Bottom Phase 4  
VOUT1a  
Amplifier 1 Output, Quadrant A  
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5
 
KAE−02150  
Table 4. PIN DESCRIPTION (continued)  
Pin  
B04  
B05  
B06  
B07  
B08  
B09  
B10  
B11  
B12  
B13  
B14  
B15  
B16  
B17  
C01  
C02  
C03  
C04  
C05  
C06  
C07  
C08  
C09  
C10  
C11  
C12  
C13  
C14  
C15  
C16  
C17  
D01  
D02  
D03  
D04  
D05  
D06  
D07  
D08  
D09  
D10  
D11  
D12  
D13  
D14  
Label  
VOUT2a  
H2SW3a  
VOUT3a  
H2BEMa  
H1Ba  
Description  
Video Output 2, Quadrant A  
HCCD Output 3 Selector, Quadrant A  
Video Output 3, Quadrant A  
EMCCD Barrier Phase 2, Quadrant A  
HCCD Barrier Phase 1, Quadrant A  
Ground  
GND  
H1Bb  
HCCD Barrier Phase 1, Quadrant B  
EMCCD Barrier Phase 2, Quadrant B  
Video Output 3, Quadrant B  
HCCD Output 3 Selector, Quadrant B  
Video Output 2, Quadrant B  
Amplifier 1 Output, Quadrant B  
VCCD Bottom Phase 4  
H2BEMb  
VOUT3b  
H2SW3b  
VOUT2b  
VOUT1b  
V4B  
SUB  
Substrate  
V1B  
VCCD Bottom Phase 1  
N/C  
No Connection  
VSS1a  
VDD23ab  
H2SW2a  
N/C  
Amplifier 1 Return, Quadrant A  
Amplifier 2 and 3 Supply, Quadrants A, B  
HCCD Output 2 Selector, Quadrant A  
No Connection  
H1SEMa  
H2Sa  
EMCCD Storage Multiplier Phase 1, Quadrant A  
HCCD Storage Phase 2, Quadrant A  
Ground  
GND  
H2Sb  
HCCD Storage Phase 2, Quadrant B  
EMCCD Storage Multiplier Phase 1, Quadrant B  
No Connection  
H1SEMb  
N/C  
H2SW2b  
VDD23ab  
VSS1b  
N/C  
HCCD Output 2 Selector, Quadrant B  
Amplifier 2 and 3 Supply, Quadrants A, B  
Amplifier 1 Return, Quadrant B  
No Connection  
V1B  
VCCD Bottom Phase 1  
V2B  
VCCD Bottom Phase 2  
VDD1a  
RG1a  
Amplifier 1 Supply, Quadrant A  
Amplifier 1 Reset, Quadrant A  
H2Xa  
Floating Gate Exit HCCD Gate, Quadrant A  
HCCD Last Gate, Outputs 1, 2 and 3, Quadrant A  
Amplifier 3 Reset, Quadrant A  
H2La  
RG3a  
H2SEMa  
H1Sa  
EMCCD Storage Multiplier Phase 2, Quadrant A  
HCCD Storage Phase 1, Quadrant A  
Ground  
GND  
H1Sb  
HCCD Storage Phase 1, Quadrant B  
EMCCD Storage Multiplier Phase 2, Quadrant B  
Amplifier 3 Reset, Quadrant B  
H2SEMb  
RG3b  
H2Lb  
HCCD Last Gate, Outputs 1, 2 and 3, Quadrant B  
Floating Gate Exit HCCD Gate, Quadrant B  
H2Xb  
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6
KAE−02150  
Table 4. PIN DESCRIPTION (continued)  
Pin  
D15  
D16  
D17  
E01  
E02  
E03  
E04  
E05  
E06  
E07  
E08  
E09  
E10  
E11  
E12  
E13  
E14  
E15  
E16  
E17  
F01  
F02  
F03  
F04  
F05  
F06  
F07  
F08  
F09  
F10  
F11  
F12  
F13  
F14  
F15  
F16  
F17  
G01  
G02  
G03  
G04  
G05  
G06  
G07  
G08  
Label  
RG1b  
VDD1b  
V2B  
Description  
Amplifier 1 Reset, Quadrant B  
Amplifier 1 Supply, Quadrant B  
VCCD Bottom Phase 2  
V2T  
VCCD Top Phase 2  
VDD1c  
RG1c  
Amplifier 1 Supply, Quadrant C  
Amplifier 1 Reset, Quadrant C  
Floating Gate Exit HCCD Gate, Quadrant C  
H2Xc  
H2Lc  
HCCD Last Gate, Outputs 1, 2 and 3, Quadrant C  
Amplifier 3 Reset, Quadrant C  
EMCCD Storage Multiplier Phase 2, Quadrant C  
HCCD Storage Phase 1, Quadrant C  
Ground  
RG3c  
H2SEMc  
H1Sc  
GND  
H1Sd  
HCCD Storage Phase 1, Quadrant D  
EMCCD Storage Multiplier Phase 2, Quadrant D  
Amplifier 3 Reset, Quadrant D  
HCCD Last Gate, Outputs 1, 2 and 3, Quadrant D  
Floating Gate Exit HCCD Gate, Quadrant D  
Amplifier 1 Reset, Quadrant D  
Amplifier 1 Supply, Quadrant D  
VCCD Top Phase 2  
H2SEMd  
RG3d  
H2Ld  
H2Xd  
RG1d  
VDD1d  
V2T  
V1T  
VCCD Top Phase 1  
N/C  
No Connection  
VSS1c  
VDD23cd  
H2SW2c  
N/C  
Amplifier 1 Return, Quadrant C  
Amplifier 2 and 3 Supply, Quadrants C, D  
HCCD Output 2 Selector, Quadrant C  
No Connection  
H1SEMc  
H2Sc  
EMCCD Storage Multiplier Phase 1, Quadrant C  
HCCD Storage Phase 2, Quadrant C  
Ground  
GND  
H2Sd  
HCCD Storage Phase 2, Quadrant D  
EMCCD Storage Multiplier Phase 1, Quadrant D  
No Connection  
H1SEMd  
N/C  
H2SW2d  
VDD23cd  
VSS1d  
N/C  
HCCD Output 2 Selector, Quadrant D  
Amplifier 2 and 3 Supply, Quadrants C, D  
Amplifier 1 Return, Quadrant D  
No Connection  
V1T  
VCCD Top Phase 1  
ESD  
ESD Protection Disable  
V4T  
VCCD Top Phase 4  
VOUT1c  
VOUT2c  
H2SW3c  
VOUT3c  
H2BEMc  
H1Bc  
Amplifier 1 Output, Quadrant C  
Video Output 2, Quadrant C  
HCCD Output 3 Selector, Quadrant C  
Video Output 3, Quadrant C  
EMCCD Barrier Phase 2, Quadrant C  
HCCD Barrier Phase 1, Quadrant C  
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7
KAE−02150  
Table 4. PIN DESCRIPTION (continued)  
Pin  
G09  
G10  
G11  
G12  
G13  
G14  
G15  
G16  
G17  
H01  
H02  
H03  
H04  
H05  
H06  
H07  
H08  
H09  
H10  
H11  
H12  
H13  
H14  
H15  
H16  
H17  
Label  
GND  
Description  
Ground  
H1Bd  
HCCD Barrier Phase 1, Quadrant D  
EMCCD Barrier Phase 2, Quadrant D  
Video Output 3, Quadrant D  
HCCD Output 3 Selector, Quadrant D  
Video Output 2, Quadrant D  
Amplifier 1 Output, Quadrant D  
VCCD Top Phase 4  
H2BEMd  
VOUT3d  
H2SW3d  
VOUT2d  
VOUT1d  
V4T  
SUB  
Substrate  
TD  
Temperature Diode Sensor  
VCCD Top Phase 3  
V3T  
N/C  
No Connection  
RG2c  
Amplifier 2 Reset, Quadrant C  
No Connection  
N/C  
VDD23cd  
H1BEMc  
H2Bc  
Amplifier 2 and 3 Supply, Quadrants C, D  
EMCCD Barrier Phase 1, Quadrant C  
HCCD Barrier Phase 2, Quadrant C  
Ground  
GND  
H2Bd  
HCCD Barrier Phase 2, Quadrant D  
EMCCD Barrier Phase 1, Quadrant D  
Amplifier 2 and 3 Supply, Quadrants C, D  
No Connection  
H1BEMd  
VDD23cd  
N/C  
RG2d  
N/C  
Amplifier 2 Reset, Quadrant D  
No Connection  
V3T  
VCCD Top Phase 3  
SUBREF  
Substrate Voltage Reference  
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8
KAE−02150  
IMAGING PERFORMANCE  
Table 5. TYPICAL OPERATIONAL CONDITIONS  
(Unless otherwise noted, the Imaging Performance Specifications are measured using the following conditions.)  
Description  
Light Source  
Condition  
Continuous Red, Green and Blue LED Illumination  
Nominal Operating Voltages and Timing  
0°C  
Notes  
1
Operation  
Temperature  
1. For monochrome sensor, only green LED used.  
Table 6. SPECIFICATIONS  
Sampling  
Plan  
Temperature  
Tested at (5C)  
Description  
Symbol  
Min.  
Nom.  
Max.  
Units  
Notes  
Dark Field Global  
Non-Uniformity  
DSNU  
2.0  
mV pp  
Die  
TBD  
TBD  
TBD  
TBD  
Bright Field Global  
Non-Uniformity  
2.0  
5.0  
1.0  
2
5.0  
15.0  
2.0  
% rms  
% pp  
% rms  
%
Die  
1
1
1
2
Bright Field Global Peak to  
Peak Non-Uniformity  
PRNU  
Die  
Bright Field Center  
Non-Uniformity  
Die  
Maximum Photoresponse  
Nonlinearity  
(EMCCD Gain = 1)  
NL  
DG  
Design  
Maximum Gain Difference  
Between Outputs  
(EMCCD Gain = 1)  
10  
1
%
%
Design  
Design  
2
2
Maximum Signal Error due  
to Nonlinearity Differences  
(EMCCD Gain = 1)  
DNL  
Horizontal CCD Charge  
Capacity  
H
Ne  
V
Ne  
P
Ne  
30  
30  
ke  
Design  
Design  
Die  
Vertical CCD Charge  
Capacity  
ke  
Photodiode Charge  
Capacity  
20  
ke  
TBD  
3
Horizontal CCD Charge  
Transfer Efficiency  
HCTE  
VCTE  
0.999995  
0.999995  
0.999999  
0.999999  
0.1  
Die  
Vertical CCD Charge  
Transfer Efficiency  
Die  
Photodiode Dark Current  
(Average)  
I
70  
e /p/s  
Die  
0
0
PD  
Vertical CCD Dark Current  
Image Lag  
6
< 1  
TBD  
Lag  
1,000  
e
Design  
Design  
Design  
Design  
Antiblooming Factor  
Vertical Smear (blue light)  
X
AB  
Smr  
−100  
9
dB  
Read Noise  
n
e rms  
4
e T  
(EMCCD Gain = 1)  
Read Noise  
(EMCCD Gain = 20)  
< 1  
1.4  
e rms  
EMCCD Excess Noise  
Factor (Gain = 20x)  
Design  
0
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9
 
KAE−02150  
Table 6. SPECIFICATIONS (continued)  
Sampling  
Plan  
Temperature  
Tested at (5C)  
Description  
Dynamic Range  
Symbol  
Min.  
Nom.  
Max.  
Units  
Notes  
DR  
68  
dB  
Design  
4, 5  
(ECCD Gain = 1)  
Dynamic Range  
(High Gain)  
60  
86  
dB  
dB  
V
Dynamic Range  
(Intra-Scene)  
Output Amplifier DC Offset  
(VOUT2, VOUT3)  
V
V
8.0  
−0.5  
10  
12.0  
2.5  
Die  
Die  
TBD  
TBD  
ODC  
ODC  
−3dB  
Output Amplifier DC Offset  
(VOUT1)  
1.0  
250  
140  
44  
V
Output Amplifier  
Bandwidth  
f
MHz  
W
Die  
6
Output Amplifier  
Impedance  
R
Die  
OUT  
Output Amplifier  
DV/DN  
mV/e  
Design  
Design  
Sensitivity (Normal output)  
Output Amplifier  
Sensitivity  
DV/DN  
(FG)  
6.2  
mV/e  
(Floating Gate Amplifier)  
Quantum Efficiency (Peak)  
Monochrome  
Red  
Green  
Blue  
QE  
%
W
Design  
Design  
MAX  
50%  
33%  
41%  
43%  
Power  
4-Output Mode  
(20MHz)  
(40MHz)  
0.8  
0.7  
2-Output Mode  
(20MHz)  
(40MHz)  
0.5  
0.5  
1-Output Mode  
(20MHz)  
(40MHz)  
0.4  
0.4  
1. Per color  
2. Value is over the range of 10% to 90% of photodiode saturation.  
3. The operating value of the substrate reference voltage, V , can be read from pin 60.  
AB  
4. At 40 MHz.  
5. Uses 20LOG (P / n ).  
Ne  
e−T  
6. Calculated from f  
= 1 / 2p R  
C  
LOAD  
where C  
= 5 pF.  
−3dB  
OUT  
LOAD  
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10  
 
KAE−02150  
TYPICAL PERFORMANCE CURVES  
Quantum Efficiency  
Monochrome with Microlens  
60  
50  
40  
30  
20  
10  
0
1,000  
300  
400  
500  
600  
700  
800  
900  
Wavelength (nm)  
Figure 5. Monochrome QE with Microlens  
Color (Bayer RGB) with Microlens  
45  
40  
35  
30  
Red  
Green  
Blue  
25  
20  
15  
10  
5
0
1,000  
350  
400  
450  
500  
550  
600  
650  
700 750  
800  
850  
900  
950  
Wavelength (nm)  
Figure 6. Color (Bayer RGB) QE with Microlens  
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11  
KAE−02150  
Angular Response  
The incident light angle is varied in a plane parallel to the HCCD.  
Monochrome with Microlens  
100  
90  
80  
70  
60  
50  
40  
30  
20  
10  
0
−30  
−20  
−10  
0
10  
20  
30  
Angle (Deg)  
Figure 7. Monochrome with Microlens Angle Response  
Color (Bayer RGB) with Microlens  
100  
90  
80  
70  
60  
50  
40  
30  
20  
10  
0
Red  
Green  
Blue  
−30  
−20  
−10  
0
10  
20  
30  
Angle (Deg)  
Figure 8. Color with Microlens Angle Response  
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12  
KAE−02150  
Frame Rates  
80  
70  
60  
50  
40  
30  
20  
10  
0
Quad  
Dual  
Single  
10  
15  
20  
25  
30  
35  
40  
Frequency (MHz)  
Figure 9. Frame Rates vs. Frequency  
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13  
KAE−02150  
DEFECT DEFINITIONS  
Table 7. DEFECT DEFINITIONS  
Description  
Threshold/Definition  
10 mV  
Maximum Number Allowed  
Notes  
Major Dark Field Defective Bright Pixel  
Major Bright Field Defective Dark Pixel  
Minor Dark Field Defective Bright Pixel  
Cluster Defect  
20  
1, 2  
12%  
5 mV  
200  
8
A Group of 2 to 10 Contiguous Major Defective  
Pixels No Greater than 2 Pixels in Width  
3
Column Defect  
A Group of More than 10 Contiguous Major  
Dark Defective Pixels along a Single Column or  
10 Contiguous Bright Defective Pixels along  
a Single Column  
0
3, 4  
1. The thresholds are defined for an operating temperature of 0°C, quad output mode, gain of 20X and a readout rate of 20 MHz. For operation  
at 22°C, thresholds of 30 mV for major bright pixels and 10 mV for minor bright pixels would give approximately the same numbers of defects.  
2. For the color device, a bright field defective pixel deviates by 12% with respect to pixels of the same color.  
3. Column and cluster defects are separated by no less than 2 good pixels in any direction (excluding single pixel defects).  
4. Low exposure dark column defects are not counted at temperatures above 0°C.  
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14  
 
KAE−02150  
OPERATION  
Table 8. ABSOLUTE MAXIMUM RATINGS  
(Absolute maximum rating is defined as a level or condition that should not be exceeded at any time per the description. If the level or the  
condition is exceeded, the device will be degraded and may be damaged. Operation at these values will reduce MTTF.)  
Description  
Operating Temperature  
Humidity  
Symbol  
Minimum  
Maximum  
Units  
°C  
Notes  
T
OP  
−70  
5
40  
90  
5
1
2
3
RH  
%
Output Bias Current  
Off-Chip Load  
I
mA  
pF  
OUT  
CL  
10  
Stresses exceeding those listed in the Maximum Ratings table may damage the device. If any of these limits are exceeded, device functionality  
should not be assumed, damage may occur and reliability may be affected.  
1. Noise performance will degrade at higher temperatures.  
2. T = 25°C. Excessive humidity will degrade MTTF.  
3. Total for all outputs. Maximum current is −15 mA for each output. Avoid shorting output pins to ground or any low impedance source during  
operation. Amplifier bandwidth increases at higher current and lower load capacitance at the expense of reduced gain (sensitivity).  
Table 9. ABSOLUTE MAXIMUM VOLTAGE RATINGS BETWEEN PINS AND GROUND  
Description  
Minimum  
−0.4  
Maximum  
17.5  
Units  
Notes  
VDD23ab, VDD23cd  
VOUT2, VOUT3  
VDD1, VOUT1  
V1B, V1T  
V
V
V
V
V
V
1
−0.4  
15  
−0.4  
7.0  
ESD – 0.4  
ESD – 0.4  
– 0.4  
ESD + 22.0  
ESD + 14.0  
10  
V2B, V2T, V3B, V3T, V4B, V4T  
H1S, H1B, H2S, H2B, H1BEM, H2BEM, H2SL, H2X,  
H2SW2, H2SW3, RG1, RG2, RG3  
1
H1SEM, H2SEM  
−0.4  
−9.0  
6.5  
20  
0.0  
40  
V
V
V
ESD  
SUB  
2, 3  
1. “a” denotes a, b, c or d.  
2. Refer to Application Note Using Interline CCD Image Sensors in High Intensity Visible Lighting Conditions.  
3. The measured value for VSUB is a diode drop higher than the recommended minimum VSUB bias.  
REF  
Power-Up and Power-Down Sequence  
SUB and ESD power up first, then power up all other  
biases in any order. No pin may have a voltage less than ESD  
at any time. All HCCD pins must be greater than or equal to  
until VDD23ab has been powered, therefore the SUB  
voltage cannot be directly derived from the SUB  
pin.  
REF  
The SUB pin should be at least 4 V before powering up  
VDD23ab or VDD23cd.  
GND at all times. The SUB  
pin will not become valid  
REF  
Table 10. DC BIAS OPERATING CONDITIONS  
Maximum  
DC Current  
Description  
Output Amplifier Return  
Output Amplifier Supply  
Output Amplifier Supply  
Ground  
Pins  
VSS1  
VDD1  
VDD23  
GND  
Symbol  
Minimum  
−8.3  
Nominal  
−8.0  
Maximum  
−7.7  
Units  
Notes  
V
SS1  
V
V
V
V
V
4 mA  
V
DD1  
4.5  
5.0  
6.0  
15 mA  
V
DD23  
+14.7  
0.0  
+15.0  
0.0  
+15.3  
0.0  
37.0 mA  
17.0 mA  
1
2
GND  
Substrate  
SUB  
V
SUB  
6.5  
VSUB  
VSUB  
REF  
+ 28  
Up to 1 mA  
(Determined by  
Photocurrent)  
REF  
− 0.5  
ESD Protection Disable  
Output Bias Current  
ESD  
ESD  
−8.3  
2.0  
−8.0  
−7.7  
5.0  
V
0.25 mA  
VOUT  
I
2.5  
mA  
OUT  
1. VDD bias pins for all four quadrants must be maintained at 15 V during operation.  
2. For each image sensor the voltage output on the VSUB pin is programmed to be one diode drop, 0.5 V, above the nominal SUB voltage.  
REF  
The voltage output on VSUB  
is unique to each image sensor and may vary from 6.5 to 10.0 V. The output impedance of VSUB  
is  
REF  
REF  
approximately 100 k. The applied VSUB should be one diode drop lower than the VSUB  
value measured on the device, when V  
REF  
DD23  
is at the specified voltage.  
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15  
 
KAE−02150  
AC Operating Conditions  
Table 11. CLOCK LEVELS  
HCCD and RG  
Low Level  
Nominal  
0.0  
Amplitude  
Low  
−0.2  
−0.2  
−0.2  
−0.2  
−0.2  
−0.2  
−0.2  
High  
0.2  
0.2  
0.2  
0.2  
0.2  
0.2  
0.2  
Low  
3.1  
3.1  
3.1  
3.1  
3.1  
3.1  
6.0  
3.1  
3.1  
4.6  
4.6  
7.0  
7.0  
Nominal  
3.3  
3.3  
3.3  
3.3  
3.3  
3.3  
6.4  
3.3  
3.3  
5.0  
5.0  
High  
3.6  
3.6  
3.6  
3.6  
3.6  
3.6  
6.8  
3.6  
3.6  
5.4  
5.4  
18.0  
18.0  
Pin  
Function  
H2B(a,b,c,d)  
Reversible HCCD Barrier 2  
Reversible HCCD Barrier 1  
Reversible HCCD Storage 2  
Reversible HCCD Storage 1  
HCCD Switch 2 and 3  
HCCD Last Gate  
H1B(a,b,c,d)  
0.0  
H2S(a,b,c,d)  
0.0  
H2B(a,b,c,d)  
0.0  
H2SW(2,3)(a,b,c,d)  
H2L(a,b,c,d)  
0.0  
0.0  
H2X(a,b,c,d)  
Floating Gate Exit  
0.0  
RG1(a,b,c,d)  
Floating Gate Reset  
Cap  
Cap  
0.0  
RG(2,3)(a,b,c,d)  
H1BEM(a,b,c,d)  
H2BEM(a,b,c,d)  
H1SEM(a,b,c,d)  
H2SEM(a,b,c,d)  
Floating Diffusion Reset  
Multiplier Barrier 1  
−0.2  
−0.2  
−0.3  
−0.3  
0.2  
0.2  
0.3  
0.3  
Multiplier Barrier 2  
0.0  
Multiplier Storage 1  
0.0  
Multiplier Storage 2  
0.0  
1. HCCD Operating Voltages. There can be no overshoot on any horizontal clock below −0.4 V: the specified absolute minimum. The H1SEM  
and H2SEM clock amplitudes need to be software programmable to adjust the charge multiplier gain.  
2. Reset Clock Operation: The RG1, RG2, and RG3 signals must be capacitive coupled into the image sensor with a 0.01 mF to 0.1 mF capacitor.  
The reset clock overshoot can be no greater than 0.3 V, as shown in Figure 10, below:  
3.1 V Minimum  
0.3 V Maximum  
Figure 10. RG Clock Overshoot  
Clock Capacitances  
Capacitance  
(pF)  
Capacitance  
(pF)  
Capacitance  
(pF)  
Capacitance  
(pF)  
Pin  
Pin  
Pin  
Pin  
H1Sa  
H1Sb  
H1Sc  
H1Sd  
H2Sa  
H2Sb  
H2Sc  
H2Sd  
76  
76  
76  
76  
76  
76  
76  
76  
H1Ba  
H1Bb  
H1Bc  
H1Bd  
H2Ba  
H2Bb  
H2Bc  
H2Bd  
39  
39  
39  
39  
39  
39  
39  
39  
H1BEMa  
H1BEMb  
H1BEMc  
H1BEMd  
H2BEMa  
H2BEMb  
H2BEMc  
H2BEMd  
56  
56  
56  
56  
56  
56  
56  
56  
H1SEMa  
H1SEMb  
H1SEMc  
H1SEMd  
H2SEMa  
H2SEMb  
H2SEMc  
H2SEMd  
66  
66  
66  
66  
66  
66  
66  
66  
NOTE: The capacitances of all other HCCD pins is 15 pF or less.  
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16  
 
KAE−02150  
H1SEMa  
H2SEMa  
High  
Low  
+18 V  
H1SEMb  
H2SEMb  
High  
Low  
A
B
4 Output  
DAC  
C
D
H1SEMc  
H2SEMc  
High  
Low  
H1SEMd  
H2SEMd  
High  
Low  
Figure 11. EMCCD Clock Adjustable Levels  
For the EMCCD clocks, each quadrant must have  
independently adjustable high levels. All quadrants have  
a common low level of GND. The high level adjustments  
must be software controlled to balance the gain of the four  
outputs.  
3.3 V  
0 to 75 W  
RG1 Clock  
Generator  
RG1  
0.01 to 0.1 mF  
3.3 V  
0 to 75 W  
RG2  
RG2,3 Clock  
Generator  
RG3  
0.01 to  
0.1 mF  
Figure 12. Reset Clock Drivers  
The reset clock drivers must be coupled by capacitors to  
the image sensor. The capacitors can be anywhere in the  
vary between 0 and 75 W depending on the layout of the  
circuit board.  
range 0.01 to 0.1 mF. The damping resistor values would  
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17  
KAE−02150  
Table 12. VCCD  
Pin  
Function  
Low  
−8.0  
−0.2  
8.5  
Nominal  
−8.0  
0
High  
−6  
V(1,2,3,4)(T,B)  
V(1,2,3,4)(T,B)  
V(1)(T,B)  
Vertical CCD Clock, Low Level  
Vertical CCD Clock, Mid Level  
0.2  
rd  
Vertical CCD Clock, High (3 ) Level  
9.0  
12.5  
1. The Vertical CCD operating voltages. The VCCD low level will be −8.0 V for operating temperatures of 0°C and above. Below 0°C the VCCD  
low level should be increased for optimum noise performance.  
Table 13. BIAS VOLTAGES  
Pin  
Function  
Low  
Nominal  
−8.0  
High  
ESD  
ESD  
−8.3  
−7.7  
SUB (Notes 1, 2)  
VDD1(a,b,c,d)  
Electronic Shutter  
VSUB  
+ 22  
VSUB  
+ 28  
REF  
REF  
Floating Gate Power  
4.5  
5.0  
6.0  
VSS1(a,b,c,d)  
Floating Gate Return  
−8.3  
14.7  
−0.5  
8.0  
−8.0  
15.0  
1.0  
−7.7  
15.3  
2.5  
VDD(2,3)(a,b,c,d)  
VOUT1(a,b,c,d)  
VOUT(2,3)(a,b,c,d)  
Floating Diffusion Power  
Floating Gate Output Range  
Floating Diffusion Output Range  
10.0  
12.0  
1. Caution: Do not clock the EMCCD register while the electronic shutter pulse is high.  
2. The substrate bias (SUB) should normally be kept at V , which can be read from Pin 60. However, this value was determined from operation  
AB  
at 0°C, and has an approximate temperature dependence of 0.01 V/degree.  
Device Identification  
The device identification pin (DevID) may be used to  
determine which ON Semiconductor 5.5 micron pixel  
interline CCD sensor is being used.  
Table 14. DEVICE IDENTIFICATION  
Maximum  
DC Current  
Description  
Pins  
Symbol  
Minimum  
Nominal  
Maximum  
Units  
Notes  
Device Identification  
DevID  
DevID  
44,000  
50,000  
56,000  
W
0.3 mA  
1, 2, 3  
1. Nominal value subject to verification and/or change during release of preliminary specifications.  
2. If the Device Identification is not used, it may be left disconnected.  
3. After Device Identification resistance has been read during camera initialization, it is recommended that the circuit be disabled to prevent  
localized heating of the sensor due to current flow through the R_DeviceID resistor.  
Recommended Circuit  
V1  
V2  
R_External  
DevID  
GND  
ADC  
R_DeviceID  
KAE−02150  
Figure 13. Device Identification Recommended Circuit  
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18  
 
KAE−02150  
THEORY OF OPERATION  
Image Acquisition  
Photo  
Diode  
Figure 14. Illustration of 2 Columns and 3 Rows of Pixels  
This image sensor is capable of detecting up to  
20,000 electrons with a small signal noise floor of 1 electron  
all within one image. Each 5.5 mm square pixel, as shown in  
Figure 14 above, consists of a light sensitive photodiode and  
a portion of the vertical CCD (VCCD). Not shown is  
a microlens positioned above each photodiode to focus light  
away from the VCCD and into the photodiode. Each photon  
incident upon a pixel will generate an electron in the  
photodiode with a probability equal to the quantum  
efficiency.  
The VCCD is shielded from light by metal to prevent  
detection of more photons. For very bright spots of light,  
some photons may leak through or around the metal light  
shield and result in electrons being transferred into the  
VCCD. This is called image smear.  
Image Readout  
At the start of image readout, the voltage on the V1T and  
V1B pins is pulsed from 0 V up to the high level for at least  
1 ms and back to 0 V, which transfers the electrons from the  
photodiodes into the VCCD. If the VCCD is not empty, then  
the electrons will be added to what is already in the VCCD.  
The VCCD is read out one row at a time. During a VCCD  
row transfer, the HCCD clocks are stopped. All gates of type  
H1 stop at the high level and all gates of type H2 stop at the  
low level. After a VCCD row transfer, charge packets of  
electrons are advanced one pixel at a time towards the output  
amplifiers by each complimentary clock cycle of the H1 and  
H2 gates.  
The charge multiplier has a maximum charge handling  
capacity (after gain) of 20,000 electrons. This is not the  
average signal level. It is the maximum signal level.  
Therefore, it is advisable to keep the average signal level at  
15,000 electrons or less to accommodate a normal  
distribution of signal levels. For a charge multiplier gain of  
20x, no more than 15,000/20 = 750 electrons should be  
allowed to enter the charge multiplier. Overfilling the charge  
multiplier beyond 20,000 electrons will shorten its useful  
operating lifetime. In addition, sending signals larger than  
180–200 electrons into the EMCCD will produce images  
with lower signal-to-noise ratio than if they were read out of  
the normal floating diffusion output. See Application Note  
AND9244.  
The photodiode may be cleared of electrons (electronic  
shutter) by pulsing the SUB pin of the image sensor up to  
a voltage of 30 V to 40 V (VSUB  
+ 22 V to VSUB  
REF  
REF  
+ 28 V) for a time of at least 1 ms. When the SUB pin is  
above 30 V, the photodiode can hold no electrons, and the  
electrons flow downward into the substrate. When the  
voltage on SUB drops below 30 V, the integration of  
electrons in the photodiode begins. The HCCD clocks  
should be stopped when the electronic shutter is pulsed, to  
avoid having the large voltage pulse on SUB coupling into  
the video outputs and altering the EMCCD gain.  
It should be noted that there are certain conditions under  
which the device will have no anti-blooming protection:  
when the V1T and V1B pins are high, very intense  
illumination generating electrons in the photodiode will  
flood directly into the VCCD. When the electronic shutter  
pulse overlaps the V1T and V1B high-level pulse that  
transfers electrons from the photodiode to the VCCD, then  
photo-electrons will flow to the substrate and not the VCCD.  
This condition may be desirable as a means to obtain very  
short integration times.  
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19  
 
KAE−02150  
To prevent overfilling the charge multiplier,  
a non-destructive floating gate output amplifier (VOUT1) is  
provided on each quadrant of the image sensor as shown in  
Figure 15.  
To VOUT2  
VOUT1  
4 Clock Cycles  
28 Clock Cycles  
1 Clock Cycle  
1 Clock  
Cycle  
10 Clock Cycles  
24 Clock Cycles  
From the Dark  
VCCD Columns  
From the Photo-Active  
VCCD Columns  
SW  
Empty Pixels  
FG  
Empty Pixels  
Charge Transfer  
2072 Clock Cycles  
To the Charge Multiplier  
and VOUT3  
Figure 15. The Charge Transfer Patch of One Quadrant  
The non-destructive floating gate output amplifier is able  
to sense how much charge is present in a charge packet  
without altering the number of electrons in that charge  
packet. This type of amplifier has a low charge-to-voltage  
The transfer sequence of a charge packet through the  
floating gate amplifier is shown in Figure 16 below.  
The time steps of this sequence are labeled A through D, and  
are indicated in the timing diagram shown as Figure 17.  
The RG1 gate is pulse high during the time that the H2X gate  
is pulsed high. This holds the floating gate at a constant  
voltage so the H2X gate can pull the charge packet out of the  
floating gate. The RG1 pulse should be at least as wide as the  
H2X pulse. The H2X pulse width should be at least 12 ns.  
The rising edge of H2X relative to the falling edge of H1S  
is critical. The H2X pulse cannot begin its rising edge  
transition until the H1S edge is less than 0.4 V. If the H2X  
rising edge comes too soon then there may be some  
backwards flow of charge for signals above  
10,000 electrons.  
conversion gain (about 6.2 mV/e ) and high noise (about  
60 electrons), but it is being used only as a threshold  
detector, and not an imaging detector. Even with  
60 electrons of noise, it is adequate to determine whether  
a charge packet is greater than or less than the recommended  
threshold of 180 electrons.  
After one row has been transferred from the VCCD into  
the HCCD, the HCCD clock cycles should begin. After 10  
clock cycles, the first dark VCCD column pixel will arrive  
at VOUT1. After another 24 (34 total) clock cycles, the first  
photo-active charge packet will arrive at VOUT1.  
VDD1  
Floating Gate Amp  
V
REF  
VOUT1  
RG1  
H2S  
H1S  
H2X  
OG1  
H2L  
H1S  
A
B
C
D
Channel  
Potential  
NOTE: The blue and green rectangles represent two separate charge packets. The direction of charge transfer is from right to left.  
Figure 16. Charge Packet Transfer Sequence through the Floating Gate Amplifier  
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20  
 
KAE−02150  
A
B
C
D
H1S  
50%  
50%  
10%  
90%  
H2S  
H2X  
10%  
RG1  
VOUT1  
Figure 17. Timing Signals that Control the Transfer of Charge through the Floating Gate Amplifier  
The charge packet is transferred under the floating gate on  
the falling edge of H2L. When this transfer takes place the  
floating gate is not connected to any voltage source.  
The presence of charge under the gate causes a change in  
voltage on the floating gate according to V = Q / C, where  
Q is the size of the charge packet and C is the capacitance of  
H2SW3 pins to route the charge packet to the charge  
multiplier. This action must take place 28 clock cycles after  
the charge packet was under the floating gate amplifier.  
The 28 clock cycle delay is to allow for pipeline delays of the  
A/D converter inside the analog front end. The timing  
generator must examine the output of the analog front end  
and dynamically alter the timing on H2SW2 and H2SW3. To  
route a charge packet to the charge multiplier (VOUT3),  
H2SW2 is held at GND and H2SW3 is clocked with the  
same timing as H2S for that one clock cycle. To route  
a charge packet to the low gain output amplifier (VOUT2),  
H2SW3 is held at GND and H2SW2 is clocked with the  
same timing as H2S for that one clock cycle.  
the floating gate. With an output sensitivity of 6.2 mV/e ,  
each electron on the floating gate would give a 6.2 mV  
change in VOUT1 voltage. Therefore if the decision  
threshold is to only allow charge packets of 180 electrons or  
less into the charge multiplier, this would correspond to  
180 × 6.2 = 1.1 mV. If the video output is less than 1.1 mV,  
then the camera must set the timing of the H2SW2 and  
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21  
KAE−02150  
EMCCD OPERATION  
H1BEM H2SEM  
H2BEM H1SEM H1BEM H2SEM H2BEM H1SEM  
A
B
C
Channel  
Potential  
D
NOTE: Charge flows from right to left.  
Figure 18. The Charge Multiplication Process  
The charge multiplication process, shown in Figure 18  
above, begins at time step A, when an electron is held under  
the H1SEM gate. The H2BEM and H1BEM gates block the  
electron from transferring to the next phase until the H2SEM  
has reached its maximum voltage. When the H2BEM is  
clocked from 0 to 5 V, the channel potential under H2BEM  
increases until the electron can transfer from H1SEM to  
H2SEM. When the H2SEM gate is above 10 V, the electric  
field between the H2BEM and H2SEM gates gives the  
electron enough energy to free a second electron which is  
collected under H2SEM. Then the voltages on H2BEM and  
H2SEM are both returned to 0 V at the same time that  
H1SEM is ramped up to its maximum voltage. Now the  
process can repeat again with charge transferring into the  
H1SEM gate.  
The alignment of clock edges is shown in Figure 19.  
The rising edge of the H1BEM and H2BEM gates must be  
delayed until the H1SEM or H2SEM gates have reached  
their maximum voltage. The falling edge of H1BEM and  
H2BEM must reach 0 V before the H1SEM or H2SEM  
reach 0 V. There are a total of 1,800 charge multiplying  
transfers through the EMCCD on each quadrant.  
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22  
 
KAE−02150  
A
B
C
D
H2S  
100%  
H2SEM  
H2BEM  
0%  
100%  
H1SEM  
H1BEM  
0%  
Figure 19. The Timing Diagram for Charge Multiplication  
The amount of gain through the EMCCD will depend on  
temperature and H1SEM and H2SEM voltage as shown in  
Figure 20. Gain also depends on substrate voltage, as shown  
in Figure 21, and on the input signal, as shown in Figure 22.  
100  
10  
0
12.0  
12.5  
13.0  
13.5  
14.0  
14.5  
15.0  
15.5  
EMCCD Voltage  
NOTE: This figure represents data from only one example image sensor, other image sensors will vary.  
Figure 20. The Variation of Gain vs. EMCCD High Voltage and Temperature  
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23  
 
KAE−02150  
15.4  
15.2  
T = 0°C  
15.0  
14.8  
14.6  
14.4  
14.2  
6
7
8
9
10  
11  
12  
13  
VSUB (V)  
NOTE: This figure represents data from only one example image sensor, other image sensors will vary.  
Figure 21. The Change in the Required EMCCD Voltage for a Gain of 20x vs. the Substrate Voltage  
22  
21  
20  
19  
18  
17  
16  
0
50  
100  
150  
200  
250  
300  
Input Signal (e)  
NOTE: The EMCCD voltage was set to provide 20x gain with an input of 180 electrons.  
Figure 22. EMCCD Gain vs. Input Signal  
If more than one output is used, then the EMCCD high  
level voltage must be independently adjusted for each  
quadrant. This is because each quadrant will require  
a slightly different voltage to obtain the same gain. In  
addition, the voltage required for a given gain differs  
unpredictably from one image sensor to the next, as in  
Figure 23. Because of this, the gain vs. voltage relationship  
must be calibrated for each image sensor, although within  
each quadrant, the H1SEM and H2SEM high level voltage  
should be equal.  
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24  
KAE−02150  
100  
10  
1
9
10  
11  
12  
13  
14  
15  
H1SEM, H2SEM High Level (V)  
Figure 23. An Example Showing How Two Image Sensors Can Have Different Gain vs. Voltage Curves  
The effective output noise of the image sensor is defined  
as the noise of the output signal divided by the gain. This is  
measured with zero input signal to the EMCCD. Figures 24  
and 25 show the EMCCD by itself has a very low noise that  
goes as the noise at gain = 1 divided by the gain. The  
EMCCD has very little clock-induced charge and does not  
require elaborate sinusoidal waveform clock drivers.  
Simple square wave clock drivers with a resistor between the  
driver and sensor for a small RC time constant are all that is  
needed. However, the pixel array may acquire spurious  
charge as a function of VCCD clock driver characteristics.  
Also, the VCCD is sensitive to hot electron luminescence  
emitted from the output amplifiers during image readout.  
These two factors limit the noise floor of the total imaging  
array.  
10  
1
0.1  
0.01  
1
10  
100  
Gain  
NOTE: This figure represents data from only one example image sensor, other image sensors will vary.  
Figure 24. EMCCD Output Noise vs. EMCCD Gain in Single Output Mode at −50 to 225C  
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25  
 
KAE−02150  
10  
1
0.1  
0.01  
1
10  
100  
Gain  
NOTE: This figure represents data from only one example image sensor, other image sensors will vary.  
Figure 25. EMCCD Output Noise vs. EMCCD Gain in Quad Output Mode at −50 to 225C  
Because of these pixel array noise sources, it is  
recommended that the maximum gain used be 40x at 0°C,  
which typically gives a noise floor between 1e and 0.4e.  
Using higher gains will provide limited benefit and will  
degrade the signal to noise ratio due to the EMCCD excess  
noise factor. Furthermore, the image sensor is not limited by  
dark current noise sources when the temperature is below  
25°C. Therefore, cooling below 25°C will not provide  
a significant improvement to the noise floor. Lower  
temperatures will reduce the number of hot pixel defects  
observed only during image integration times longer than  
1 s. Note the useful plot below:  
1,000  
100  
10  
1
13.0  
13.5  
14.0  
14.5  
15.0  
15.5  
EMCCD Voltage  
CAUTION: The EMCCD should not be operated near saturation for an extended period, as this may result in gain aging and  
permanently reduce the gain. It should be noted that device degradation associated with gain aging is not covered under  
the device warranty.  
Figure 26. Gain vs. Voltage with Maximum Recommended Operating Gains Marked  
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26  
KAE−02150  
Choosing the Operating Temperature  
The reasons for lowering the operating temperature are to  
reduce dark current noise and to reduce image defects.  
The average dark signal from the VCCD and photodiodes  
must be less than 1e in order to have a total system noise less  
than 1e when using the EMCCD. Figures 27 and 28 illustrate  
how the amount of dark signal in the VCCD is dependent on  
both temperature and voltage, and may be used to choose the  
operating temperature and VCCD clock low level voltage.  
When operating in quad output mode at 0°C either −6 V  
or −8 V may be used for the VCCD clock low level voltage  
because the dark signal will be equal. But if the operating  
temperature is −20°C then the VCCD clock low level  
voltage should be set to −6 V for the lowest VCCD dark  
signal. For single output mode, the VCCD clock low level  
voltage should be set to −6 V for temperatures of −10°C or  
lower and −8 V for temperatures of −10°C or higher.  
1.0  
0.8  
0.6  
0.4  
0.2  
0.0  
−50  
−40  
−30  
−20  
−10  
0
10  
20  
Temperature (5C)  
NOTE: Both are for a HCCD frequency of 20 MHz. The VCCD low level voltage is shown for each curve.  
Figure 27. Dark Signal from VCCD in Quad and Single Output Modes  
1.0  
0.8  
0.6  
0.4  
0.2  
0.0  
−50  
−40  
−30  
−20  
−10  
0
10  
20  
Temperature (5C)  
Figure 28. Dark Signal from VCCD in Dual Output Mode at HCCD Frequency 20 MHz  
The reason for the different temperature dependencies  
with the VCCD low level voltage at −6 V vs. −8 V is spurious  
charge generation (sometimes called clock-induced charge).  
When the VCCD low level is at −8 V, the VCCD is  
accumulated with holes, which reduces the rate of dark  
current signal generation. However, the amount of clock  
induced charge is greater. At VCCD low level of −6 V,  
the VCCD is no longer accumulated with holes. So,  
clock-induced charge generation is less, but dark current is  
increased.  
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27  
 
KAE−02150  
In quad output mode, the clock induced charge generated  
In addition to dark noise, image defects also impact the  
optimum operating temperature. Although the average  
photodiode dark current is negligible at temperatures below  
20°C, as shown by Figure 29, the number of photodiode  
hot-pixel defects is a function of temperature and will  
decrease with lower temperature.  
and the dark current signal are equal at T = 0°C. Below  
T = 0°C, the dark current signal is smaller than the clock  
induced charge, so −6 V is the best voltage. Above T = 0°C,  
the dark current signal dominates, and −8 V is the best  
voltage. The dark signal stops decreasing below T = −20°C  
because the VCCD is detecting hot electron luminescence  
from the output amplifiers during image readout.  
0.1000  
0.0100  
0.0010  
0.0001  
−30  
−20  
−10  
0
10  
20  
Temperature (5C)  
Figure 29. Photodiode Dark Current vs. Temperature  
Note that the preceding figures are representative data  
only, and are not intended as a defect specification.  
to at least 3 times the floating gate amplifier noise, or 180 e .  
Sending signals larger than 180 e into the EMCCD will  
produce images with lower S/N than if they were read out of  
the normal floating diffusion output of VOUT2. See  
Application Note AND9244.  
Choosing the Charge Switch Threshold  
The floating gate output amplifier (VOUT1) is used to  
decide the routing of a pixel at the charge switch. Pixels with  
large signals should be routed to the normal floating  
diffusion amplifier at VOUT2. Pixels with small signals  
should be routed to the EMCCD and VOUT3. The routing  
of pixels is controlled by the timing on H2SW2 and H2SW3.  
The optimum signal threshold for that transition between  
VOUT2 and VOUT3 is when the signal to noise ratio (S/N)  
of VOUT2 is equal to the S/N of VOUT3. This signal is  
given by  
Temperature Diode  
There is a diode integrated on the same silicon die as the  
image sensor that can be used to assist temperature  
regulation. It is not accurate enough to provide a calibrated  
temperature value, but it can be used to maintain a constant  
temperature.  
The temperature is sensed by forward biasing the diode  
with 50 mA of current and measuring the resulting voltage  
drop. The current value most preferred is 50 mA. It is  
recommended that it not be less than 40 mA or more than  
60 mA.  
The primary source of inaccuracy in temperature  
measurement is noise contributed by other clock inputs to  
the image sensor. The small amount of coupling of the other  
clocks to the temperature diode is rectified by the  
temperature diode and causes an offset error in the voltage  
reading. The magnitude of the offset error is dependent upon  
factors such as the number of outputs used, and the layout of  
the camera circuit board. While the error frustrates obtaining  
G ) 1  
S + s2T  
@
(eq. 1)  
G
where G is the EMCCD gain, S is the signal level, and s is  
T
the total system noise on VOUT2 in the dark. For values of  
G greater than 10, the optimum signal threshold occurs when  
then signal equals the square of the total system noise floor  
s . Depending on the skill of the camera designer, s will  
T
T
range from 8 to 12 e . If the camera has a total system noise  
of 10 e , then the threshold should be set to 100 e . However,  
the floating gate amplifier noise is approximately 60 e−, and  
so would dominate, making it preferable to set the threshold  
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28  
 
KAE−02150  
an accurate absolute temperature value, it is expected to be  
constant and allow the diode to be used for maintaining  
a constant temperature.  
Figure 30 shows the forward biased voltage drop across  
the diode vs. temperature with a current of 50 mA. There are  
two curves showing the offset error. One curve shows the  
temperature dependence with all image sensor clocks  
stopped, and the second with all clocks operating at 20 MHz,  
The offset between the clocks-on and clocks-off curves will  
be different for every camera design.  
−0.55  
−0.60  
−0.65  
−0.70  
−0.75  
−0.80  
−0.85  
−50  
−40  
−30  
−20  
−10  
0
10  
20  
30  
40  
50  
Temperature (5C)  
NOTE: The “clocks on” voltage curve will vary significantly from one camera design to the next.  
Figure 30. Voltage Drop across Temperature Sensing Diode with Current of 50 mA  
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29  
 
KAE−02150  
TIMING DIAGRAMS  
Pixel Timing  
50 ns  
H2S, H2L  
H1S  
H2X  
RG1  
RG2  
H2SEM  
H2BEM  
H1SEM  
H1BEM  
NOTE: The minimum time for one pixel is 50 ns.  
Figure 31. Pixel Timing Pattern P1  
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30  
KAE−02150  
Black Clamp, VOUT1, VOUT2, and VOUT3 Alignment  
at Line Start  
VOUT3 on the same clock cycle and exactly two rows after  
they would have arrived at VOUT2.Changing the number of  
HCCD clock cycles with introduce an offset between when  
pixels arrive at VOUT2 or VOUT3.  
When in single mode, each row must have exactly 2,072  
HCCD clock cycles. The pixels arrive at VOUT3 on the  
same clock cycle and exactly one row after they would have  
arrived at VOUT2.Changing the number of HCCD clock  
cycles with introduce an offset between when pixels arrive  
at VOUT2 or VOUT3.  
The black level clamp should start 3 clock cycles into the  
line and be active for 28 clock cycles of each row. The first  
photoactive pixel will arrive at the VOUT1 (floating gate)  
output after 34 clock cycles. The first photoactive pixel will  
arrive at either the VOUT2 or VOUT3 after 68 clock cycles,  
depending on the timing of H2SW2 and H2SW3.  
When in dual or quad output mode, each row must have  
exactly 1,036 HCCD clock cycles. The pixels arrive at  
Black Clamp  
H2L  
VOUT1  
VOUT2, VOUT3  
active pixel 1  
68 pixels  
34 pixels  
active pixel 1  
1036 H2L clock cycles  
28 pixels  
0.0  
0.5  
1.0  
1.5  
2.0  
Time (ms)  
2.5  
3.0  
3.5  
4.0  
Figure 32. Video Output at Each Line Start  
H2L, VOUT1, VOUT2, and VOUT3 Alignment at End of  
Line  
output mode, the pixels arrive at VOUT3 one line delayed  
from when they would have arrived at VOUT2. When in  
dual or quad output modes, the pixels arrive at VOUT3 two  
lines delayed from when they would have arrived at  
VOUT2.  
The last active pixel (the center column of the image),  
th  
arrives at VOUT2 or VOUT3 on the 1,036 clock cycle of  
the HCCD. The last photoactive pixel arrives at VOUT1 34  
clock cycles before VOUT2 or VOUT3. When in single  
H2L  
VOUT1  
VOUT2, VOUT3  
active pixel 968  
active pixel 968  
34 pixels  
H2L clock cycle 1036  
0.0  
0.5  
1.0  
1.5  
2.0  
2.5  
3.0  
3.5  
4.0  
Time (ms)  
Figure 33. Video Output at End of Each Line for Dual or Quad Output Modes  
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31  
KAE−02150  
VCCD Timing  
Table 15. TIMING DEFINITIONS  
Symbol  
Note  
Minimum  
Nominal  
0.50  
1.30  
1.5  
Maximum  
0.50  
Units  
ms  
t
VA  
VCCD Transfer Time A  
0.46  
0.46  
1.0  
t
VB  
VCCD Transfer Time B  
7.50  
ms  
t
Electronic Shutter Pulse  
10.0  
ms  
SUB  
t
3
Photodiode to VCCD Transfer Time  
1.0  
1.5  
5.0  
ms  
V1, V2, V3, V4 Alignment  
V1B, V1T  
V2B, V4T  
V3B, V3T  
V4B, V2T  
t
VB  
t
VB  
t
3
t
VB  
t
VB  
t
VB  
t
VA  
t
VA  
t
VA  
t
VA  
Figure 34. Timing Pattern F1. VCCD Frame Timing to Transfer Charge from Photodiodes to the VCCD  
when Using the Bottom HCCD, Outputs A or B  
V1B  
V2B, V3T  
V3B, V4T  
V4B  
V1T  
V2T  
t
VB  
t
VB  
t
3
t
VB  
t
VB  
t
VB  
t
VA  
t
VA  
t
VA  
t
VA  
Figure 35. Timing Pattern F2. VCCD Frame Timing to Transfer Charge from Photodiodes to the VCCD  
when Using All Four Outputs in Quad Mode  
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32  
KAE−02150  
V1B, V1T  
V2B, V4T  
V3B, V3T  
V4B, V2T  
t
VB  
t
VB  
t
VB  
t
VB  
t
VA  
t
VA  
t
VA  
t
VA  
Figure 36. Line Timing L1. VCCD Line Timing to Transfer One Line of Charge from VCCD to the HCCD  
when Using the Bottom HCCD, Outputs A or B in Single or Dual Output Modes  
V1B, V2T  
V2B, V3T  
V3B, V4T  
V4B, V1T  
t
VB  
t
VB  
t
VB  
t
VB  
t
VA  
t
VA  
t
VA  
t
VA  
Figure 37. Line Timing L2. VCCD Line Timing to Transfer One Line of Charge from VCCD to the HCCD  
when Using All Four Outputs in Quad Mode  
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33  
KAE−02150  
Electronic Shutter  
V
AB  
+ V  
ES  
VSUB  
V
AB  
3.3 V  
0 V  
HCCD  
VCCD  
0 V  
−8 V  
t
VB  
t
t
VB  
SUB  
Last HCCD  
Clock Edge  
First VCCD  
Clock Edge  
CAUTION: Do not clock the EMCCD register while the electronic shutter pulse is high.  
Figure 38. Electronic Shutter Timing Pattern S1  
Clock  
State  
H1S  
High  
H2S  
H2SW  
H2L  
Low  
Low  
Low  
Low  
High  
High  
Low  
Low  
H2X  
H1SEM  
H1BEM  
H2SEM  
H2BEM  
Figure 39. The State of the HCCD and EMCCD Clocks during the Frame, Line,  
and Electronic Shutter Timing Sequences  
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34  
KAE−02150  
HCCD Timing  
To reverse the direction of charge transfer in a Horizontal  
CCD, exchange the timing pattern of the H1B and H2B  
inputs of that HCCD. If a HCCD is not used, hold all of its  
gates at the high level.  
When operating in single or dual output modes,  
the VDD23cd, VDD1c, and VDD1d amplifiers must still be  
powered. The outputs VOUT1, VOUT2, and VOUT3 for  
quadrants c and d may be left unloaded.  
Table 16. HCCD TIMING  
Mode  
HCCD a, b Timing  
H1Ba = H2Bb = H1Sa = H1Sb  
HCCD c, d Timing  
Single  
3.3 V  
H2Ba = H1Bb = H2Sa = H2Sb  
Dual  
H1Ba = H1Bb = H1Sa = H1Sb  
H2Ba = H2Bb = H2Sa = H2Sb  
3.3 V  
Quad  
H1Ba = H1Bb = H1Sa = H1Sb  
H2Ba = H2Bb = H2Sa = H2Sb  
H1Bc = H1Bd = H1Sc = H1Sd  
H2Bc = H2Bd = H2Sc = H2Sd  
Image Exposure and Readout  
The flowchart for image exposure and readout is shown in  
Figure 40. The electronic shutter timing may be omitted to  
obtain an exposure time equal to the image read out time.  
NEXP is the number of lines exposure time and NV is the  
number of VCCD clock cycles (row transfers).  
Table 17. IMAGE EXPOSURE AND READOUT  
Mode  
Single  
Dual  
NH  
NV  
1,124  
562  
Line Timing  
Frame Timing  
Pixel Timing  
2,072  
1,036  
1,036  
L1  
L1  
L2  
F1  
F1  
F2  
P1  
P1  
P1  
Quad  
562  
Frame Timing  
Line Timing  
Pixel Timing  
Line Timing  
Pixel Timing  
Repeat NH Times  
Repeat NH Times  
Repeat NV − NEXP  
Times  
Repeat NEXP Times  
Electronic  
Shutter Timing  
Figure 40. The Image Readout Timing Flow Chart  
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35  
 
KAE−02150  
Long Integrations and Readout  
output SUBV will be invalid. For cameras with long  
integration times, the value of SUBV will have to digitized  
by and ADC and stored at the time when VDD23 is +15 V.  
The SUB pin voltage would be set by a DAC. The HCCD  
and EMCCD may be continue to clock during integration.  
If they are stopped during integration then the EMCCD  
should be re-started at +7 V to flush out any undesired signal  
before increasing the voltage to charge multiplying levels.  
The timing flow chart for long integration time is shown  
in Figure 41.  
For extended integrations the output amplifiers need to be  
powered down. When powered up, the output amplifiers  
emit near infrared light that is sensed by the photodiodes. It  
will begin to be visible in images of 30 second integrations  
or longer.  
To power down the output amplifiers set VDD1 and VSS1  
to 0 V, and VDD23 to +5 V. Do not set VDD23 to 0 V during  
the integration of an image. During the time the VDD2  
supply is reduced to +5 V the substrate voltage reference  
Stop All VCCD Clocks at  
the V (−8 V) Level.  
LOW  
Pulse the Electronic Shutter on VSUB  
to Empty All Photodiodes.  
Integration Begins on the Falling Edge  
of the Electronic Shutter Pulse.  
Set VDD23 = +5.0 V  
Set VDD1 = 0.0 V  
Set VSS1 = 0.0 V  
Wait…  
Set VDD23 = +15.0 V  
Set VDD1 = +5.0 V  
Set VSS1 = −8.0 V  
Begin Normal Line Timing  
Repeat for at Least 2,048 Lines  
in Single or Dual Output Mode,  
1,024 Lines in Quad Output  
Mode.  
Readout the Photodiodes  
and One Image.  
Figure 41. Timing Flow Chart for Long Integration Time  
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36  
 
KAE−02150  
STORAGE AND HANDLING  
Table 18. STORAGE CONDITIONS  
Description  
Storage Temperature  
Humidity  
Symbol  
Minimum  
Maximum  
Units  
°C  
Notes  
T
ST  
−55  
5
80  
90  
1
2
RH  
%
1. Long-term storage toward the maximum temperature will accelerate color filter degradation.  
2. T = 25°C. Excessive humidity will degrade Mean Time to Failure (MTTF).  
For information on ESD and cover glass care and  
cleanliness, please download the Image Sensor Handling  
and Best Practices Application Note (AN52561/D) from  
www.onsemi.com.  
For quality and reliability information, please download  
the Quality & Reliability Handbook (HBD851/D) from  
www.onsemi.com.  
For information on device numbering and ordering codes,  
please download the Device Nomenclature technical note  
(TND310/D) from www.onsemi.com.  
For information on environmental exposure, please  
download the Using Interline CCD Image Sensors in High  
Intensity Lighting Conditions Application Note  
(AND9183/D) from www.onsemi.com.  
For information on Standard terms and Conditions of  
Sale, please download Terms and Conditions from  
www.onsemi.com.  
For information on soldering recommendations, please  
download the Soldering and Mounting Techniques  
Reference  
Manual  
(SOLDERRM/D)  
from  
www.onsemi.com.  
www.onsemi.com  
37  
 
KAE−02150  
MECHANICAL INFORMATION  
PGA Completed Assembly  
Notes:  
1. Substrate is a 141-pin ceramic PGA package.  
2. Body is black alumina.  
3. Pins are Kovar or equivalent, plated with 1.00 microns of gold over 2.00 microns of nickel.  
4. Wire is wedge bonded aluminum (1% Si).  
5. Ablebond 967−1 epoxy for die attach.  
6. No materials to obstruct the clearance through the package holes.  
7. Exposed metal is 1.00 micron minimum gold over 2.00 micron minimum nickel.  
8. Glass lid is Schott E263Teco, n 1.5231. Thickness 0.76 0.05 mm.  
D
9. Recommended mounting screws: 1.6 × 0.35 mm (ISO standard), 0−80 (unified fine thread standard).  
Figure 42. Completed Assembly (1/2)  
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38  
KAE−02150  
Notes:  
1. Die is standard thickness for 150 mm silicon wafer: 0.675 0.020 mm.  
2. Singulated die is approximately 12.910 × 8.500 mm, for a 50 micron saw kerf.  
3. The optical center of the image area is at the center of the die and the center of the package.  
Figure 43. Completed Assembly (2/2)  
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39  
KAE−02150  
PGA Clear Cover Glass  
Notes:  
1. Dust and Scratch: 10 micron maximum (“A” zone)  
2. Glass Material: Schott D263T eco  
Figure 44. PGA Clear Cover Glass  
ON Semiconductor and the  
are registered trademarks of Semiconductor Components Industries, LLC (SCILLC) or its subsidiaries in the United States and/or other countries.  
SCILLC owns the rights to a number of patents, trademarks, copyrights, trade secrets, and other intellectual property. A listing of SCILLC’s product/patent coverage may be accessed  
at www.onsemi.com/site/pdf/Patent−Marking.pdf. SCILLC reserves the right to make changes without further notice to any products herein. SCILLC makes no warranty, representation  
or guarantee regarding the suitability of its products for any particular purpose, nor does SCILLC assume any liability arising out of the application or use of any product or circuit, and  
specifically disclaims any and all liability, including without limitation special, consequential or incidental damages. “Typical” parameters which may be provided in SCILLC data sheets  
and/or specifications can and do vary in different applications and actual performance may vary over time. All operating parameters, including “Typicals” must be validated for each  
customer application by customer’s technical experts. SCILLC does not convey any license under its patent rights nor the rights of others. SCILLC products are not designed, intended,  
or authorized for use as components in systems intended for surgical implant into the body, or other applications intended to support or sustain life, or for any other application in which  
the failure of the SCILLC product could create a situation where personal injury or death may occur. Should Buyer purchase or use SCILLC products for any such unintended or  
unauthorized application, Buyer shall indemnify and hold SCILLC and its officers, employees, subsidiaries, affiliates, and distributors harmless against all claims, costs, damages, and  
expenses, and reasonable attorney fees arising out of, directly or indirectly, any claim of personal injury or death associated with such unintended or unauthorized use, even if such claim  
alleges that SCILLC was negligent regarding the design or manufacture of the part. SCILLC is an Equal Opportunity/Affirmative Action Employer. This literature is subject to all applicable  
copyright laws and is not for resale in any manner.  
PUBLICATION ORDERING INFORMATION  
LITERATURE FULFILLMENT:  
N. American Technical Support: 800−282−9855 Toll Free  
USA/Canada  
Europe, Middle East and Africa Technical Support:  
Phone: 421 33 790 2910  
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Phone: 81−3−5817−1050  
ON Semiconductor Website: www.onsemi.com  
Order Literature: http://www.onsemi.com/orderlit  
Literature Distribution Center for ON Semiconductor  
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Phone: 303−675−2175 or 800−344−3860 Toll Free USA/Canada  
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Email: orderlit@onsemi.com  
For additional information, please contact your local  
Sales Representative  
KAE−02150/D  

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