KAI-2001-ABA-CP-BA - ON Semiconductor

February, 2016 − Rev. 3 1Publication Order Number:

KAI−2001/D

KAI-2001

1600 (H) x 1200 (V) Interline

CCD Image Sensor

Description

The KAI−2001 Image Sensor is a high-performance 2-million pixel

sensor designed for a wide range of medical, scientific and machine

vision applications. The 7.4 mm square pixels with microlenses

provide high sensitivity and the large full well capacity results in high

dynamic range. The split horizontal register offers a choice of single or

dual output allowing either 15 or 30 frame per second (fps) video rate

for the progressively scanned images. Also included is a fast line

dump for sub-sampling at higher frame rates. The vertical overflow

drain structure provides anti-blooming protection and enables

electronic shuttering for precise exposure control. Other features

include low dark current, negligible lag and low smear.

Table 1. GENERAL SPECIFICATIONS

Parameter Typical Value

Architecture Interline CCD, Progressive Scan

Total Number of Pixels 1640 (H) × 1214 (V)

Number of Effective Pixels 1608 (H) × 1208 (V)

Number of Active Pixels 1600 (H) × 1200 (V)

Pixel Size 7.4 mm (H) × 7.4 mm (V)

Active Image Size 13.38 mm (H) × 9.52 mm (V),

14.803 mm (Diagonal),

1″ Optical Format

Aspect Ratio 4:3

Number of Outputs 1 or 2

Saturation Signal 40,000 e−

Quantum Efficiency

−ABA

−CBA (RGB) 55%

45%, 42%, 35%

Output Sensitivity 16 mV/e−

Total System Noise

40 MHz

20 MHz 40 e−

23 e−

Dark Current < 0.5 nA/cm2

Dark Current Doubling Temp. 7°C

Dynamic Range 60 dB

Charge Transfer Efficiency > 0.999999

Blooming Suppression 300X

Smear 80 dB

Image Lag < 10 e−

Maximum Data Rate 40 MHz

Package 32-pin, CERDIP

NOTE: All Parameters are specified at T = 40°C unless otherwise noted.

Features

•High Resolution

•High Sensitivity

•High Dynamic Range

•Low Noise Architecture

•High Frame Rate

•Binning Capability for Higher Frame Rate

•Electronic Shutter

Applications

•Machine Vision

•Scientific

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Figure 1. KAI−2001 Interline CCD

Image Sensor

See detailed ordering and shipping information on page 2 o

this data sheet.

ORDERING INFORMATION

KAI−2001

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ORDERING INFORMATION

Table 2. ORDERING INFORMATION − KAI−2001 IMAGE SENSOR

Part Number Description Marking Code

KAI−2001−AAA−CF−BA Monochrome, No Microlens, CERDIP Package (Sidebrazed),

Quartz Cover Glass (No Coatings), Standard Grade KAI−2001

Serial Number

KAI−2001−AAA−CF−AE Monochrome, No Microlens, CERDIP Package (Sidebrazed),

Quartz Cover Glass (No Coatings), Engineering Sample

KAI−2001−AAA−CP−BA Monochrome, No Microlens, CERDIP Package (Sidebrazed),

Taped Clear Cover Glass, Standard Grade

KAI−2001−AAA−CP−AE Monochrome, No Microlens, CERDIP Package (Sidebrazed),

Taped Clear Cover Glass, Engineering Sample

KAI−2001−AAA−CR−BA* Monochrome, No Microlens, CERDIP Package (Sidebrazed),

Taped Clear Cover Glass with AR Coating (2 Sides), Standard Grade

KAI−2001−AAA−CR−AE* Monochrome, No Microlens, CERDIP Package (Sidebrazed),

Taped Clear Cover Glass with AR Coating (2 Sides), Engineering Sample

KAI−2001−ABA−CD−BA Monochrome, Telecentric Microlens, CERDIP Package (Sidebrazed),

Clear Cover Glass with AR Coating (Both Sides), Standard Grade KAI−2001M

Serial Number

KAI−2001−ABA−CD−AE Monochrome, Telecentric Microlens, CERDIP Package (Sidebrazed),

Clear Cover Glass with AR Coating (Both Sides), Engineering Sample

KAI−2001−ABA−CP−BA Monochrome, Telecentric Microlens, CERDIP Package (Sidebrazed),

Taped Clear Cover Glass, Standard Grade

KAI−2001−ABA−CP−AE Monochrome, Telecentric Microlens, CERDIP Package (Sidebrazed),

Taped Clear Cover Glass, Engineering Sample

KAI−2001−CBA−CD−BA* Color Gen1 (Bayer RGB), Telecentric Microlens, CERDIP Package (Sidebrazed),

Clear Cover Glass with AR Coating (Both Sides), Standard Grade KAI−2001CM

Serial Number

KAI−2001−CBA−CD−AE* Color Gen1 (Bayer RGB), Telecentric Microlens, CERDIP Package (Sidebrazed),

Clear Cover Glass with AR Coating (Both Sides), Engineering Sample

*Not recommended for new designs.

Table 3. ORDERING INFORMATION − EVALUATION SUPPORT

Part Number Description

KAI−2020−12−20−A−EVK Evaluation Board, 12 Bit, 20 MHz (Complete Kit)

KAI−2020−10−40−A−EVK Evaluation Board, 10 Bit, 40 MHz (Complete Kit)

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.

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DEVICE DESCRIPTION

Architecture

Figure 2. Sensor Architecture

1600 (H) x 1200 (V)

Active Pixels

BGG

Pixel

1,1

4 Buffer Rows

2 Dark Rows

4 Buffer Columns

16 Dark Columns

4 Dummy Pixels

Dual

Video L Video R

4 16 4 1600 4 16 4

Single

4 16 4 800 800 4 16 4

Output

4 Buffer Rows

4 Dark Rows

4 Buffer Columns

16 Dark Columns

There are 2 light shielded rows followed 1,208

photoactive rows and finally 4 more light shielded rows.

The first 4 and the last 4 photoactive rows are buffer rows

giving a total of 1,200 lines of image data.

In the single output mode all pixels are clocked out of the

Video L output in the lower left corner of the sensor. The first

4 empty pixels of each line do not receive charge from the

vertical shift register. The next 16 pixels receive char ge from

the left light shielded edge followed by 1,608 photosensitive

pixels and finally 16 more light shielded pixels from the

right edge of the sensor. The first and last 4 photosensitive

pixels are buffer pixels giving a total of 1,600 pixels of

image data.

In the dual output mode the clocking of the right half of the

horizontal CCD is reversed. The left half of the image is

clocked out V ideo L and the right half of the image is clocked

out Video R. Each row consists of 4 empty pixels followed

by 16 light shielded pixels followed by 800 photosensitive

pixels. When reconstructing the image, data from Video R

will have to be reversed in a line buf fer and appended to the

Video L data.

There are 4 dark reference rows at the top and 2 dark rows

at the bottom of the image sensor. The dark rows are not

entirely dark and so should not be used for a dark reference

level. Use the 16 dark columns on the left or right side of the

image sensor as a dark reference.

Of the 16 dark columns, the first and last dark columns

should not be used for determining the zero signal level.

Some light does leak into the first and last dark columns.

Only use the center 14 columns of the 16 column dark

reference.

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Pixel

ÉÉÉÉÉÉÉÉÉ

Figure 3. Pixel Architecture

Top View

Direction

Charge

Transfer

True Two Phase Burried Channel VCCD

Lightshield over VCCD not shown

Photodiode

Transfer

Gate

ËËËËË

Direction of

Charge

Transfer

ÉÉ

ÏÏÏÏÏÏ

ÉÉ

ÏÏÏÏÏÏÏ

ÉÉ

ËËËËË

n− n

n− n−

p Well (GND)

Cross Section Down Through VCCD

n Substrate

Light Shield

Cross Section Through

Photodiode and VCCD Phase 1

Photodiode

Light Shield

n Substrate

Cross Section Through Photodiode

and VCCD Phase 2 at Transfer Gate

Transfer

Gate

Cross Section Showing Lenslet

Lenslet

VCCD VCCD

Light Shield Light Shield

Photodiode

Red Color Filter

NOTE: Drawings not scale.

7.4 mm

n Substrate

An electronic representation of an image is formed when

incident photons falling on the sensor plane create

electron-hole pairs within the individual silicon

photodiodes. These photoelectrons are collected locally by

the formation of potential wells at each photosite. 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.

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Vertical to Horizontal Transfer

Figure 4. Vertical to Horizontal Transfer Architecture

ÉÉÉÉÉÉ

Top View

Direction of

Vertical

Charge

ÉÉÉÉÉÉÉÉÉÉ

Transfer

ËËËËËË

ÉÉÉÉÉÉÉÉÉÉ

Photodiode

ËËËËËË

Transfer

Gate

ËËËËËË

Fast

Line

Dump

H1S

ËË

Direction of

Horizontal

Charge Transfer

Lightshield

Not Shown

H2B

H2S

H1B

When the V1 and V2 timing inputs are pulsed, charge in

every pixel of the VCCD is shifted one row towards the

HCCD. The last row next to the HCCD is shifted into the

HCCD. When the VCCD is shifted, the timing signals to the

HCCD must be stopped. H1 must be stopped in the high state

and H2 must be stopped in the low state. The HCCD

clocking may begin tHD ms after the falling edge of the V1

and V2 pulse.

Charge i s transferred from the last vertical CCD phase into

the H1S horizontal CCD phase. Refer to Figure 27 for an

example of timing that accomplishes the vertical to

horizontal transfer of charge.

If the fast line dump is held at the high level (FDH) during

a vertical to horizontal transfer, then the entire line is

removed and not transferred into the horizontal register.

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Horizontal Register to Floating Diffusion

Figure 5. Horizontal Register to Floating Diffusion Architecture

R OG H2B H1B H2S H2B H1S H1BRD

ÏÏ

ÏÏÏ

ÏÏÏÏ

H1S

Floating

Diffusion

n (burried channel)

nn+

p (GND)

n (SUB)

n− n− n−n−

The HCCD has a total of 1,648 pixels. The 1,640 vertical

shift registers (columns) are shifted into the center 1,640

pixels of the HCCD. There are 4 pixels at both ends of the

HCCD, which receive no charge from a vertical shift

pixels (containing no electrons). The next 16 clock cycles

will contain only electrons generated by dark current in the

VCCD and photodiodes. The next 1,608 clock cycles will

contain photo-electrons (image data). Finally, the last 16

clock cycles will contain only electrons generated by dark

current in the VCCD and photodiodes. Of the 16 dark

columns, the first and last dark columns should not be used

for determining the zero signal level. Some light does leak

into the first and last dark columns. Only use the center 14

columns of the 16 column dark reference.

When the HCCD is shifting valid image data, the timing

inputs to the electronic shutter (SUB), VCCD (V1, V2),

and fast line dump (FD) should be not be pulsed. This

prevents unwanted noise from being introduced. The HCCD

is a type of charge coupled device known as a pseudo-two

phase CCD. This type of CCD has the ability to shift charge

in two directions. This allows the entire image to be shifted

out to the video L output, or to the video R output (left/right

image reversal). The HCCD is split into two equal halves of

824 pixels each. When operating the sensor in single output

mode the two halves of the HCCD are shifted in the same

direction. When operating the sensor in dual output mode

the two halves of the HCCD are shifted in opposite

directions. The direction of charge transfer in each half is

controlled by the H1BL, H2BL, H1BR, and H2BR timing

inputs.

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Horizontal Register Split

Figure 6. Horizontal Register

Single Output

H2SL

H1SL H1BL H2SRH1SR H2BR

H1BR

Pixel

824 Pixel

825

H2SL H2BLH1BL

H1 H1 H1 H1 H1H2 H2 H2 H2 H2

H2SL

H1SL H1BL H2SRH1SR H2BR

H1BR

Pixel

824 Pixel

825

H2SL H2BLH1BL

H1 H1 H1 H1 H2H2 H2 H2 H1 H2

Dual Output

Single Output Operation

When operating the sensor in single output mode all pixels

of the image sensor will be shifted out the Video L output

(pin 31). To conserve power and lower heat generation the

output amplifier for Video R may be turned off by

connecting VDDR (pin 24) and VOUTR (pin 24) to GND

(zero volts).

The H1 timing from the timing diagrams should be

applied to H1SL, H1BL, H1SR, H2BR, and the H2 timing

should be applied to H2SL, H2BL, H2SR, and H1BR. In

other words, the clock driver generating the H1 timing

should b e connected to pins 4, 3, 13, and 15. The clock driver

generating the H2 timing should be connected to pins 5, 2,

12, and 14. The horizontal CCD should be clocked for 4

empty pixels plus 16 light shielded pixels plus 1,608

photoactive pixels plus 16 light shielded pixels for a total o f

1,644 pixels.

Dual Output Operation

In dual output mode the connections to the H1BR and

H2BR pins are swapped from the single output mode to

change the direction of charge transfer of the right side

horizontal shift register. In dual output mode both VDDL

and VDDR (pins 25, 24) should be connected to 15 V.

The H1 timing from the timing diagrams should be applied

to H1SL, H1BL, H1SR, H1BR, and the H2 timing should be

applied t o H2SL, H2BL, H2SR, and H2BR. The clock driver

generating the H1 timing should be connected to pins 4, 3,

13, and 14. The clock driver generating the H2 timing should

be connected to pins 5, 2, 12, and 15. The horizontal CCD

should be clocked for 4 empty pixels plus 16 light shielded

pixels plus 804 photoactive pixels for a total of 824 pixels.

If the camera is to have the option of dual or single output

mode, the clock driver signals sent to H1BR and H2BR may

be swapped by using a relay. Another alternative is to have

two extra clock drivers for H1BR and H2BR and invert the

signals in the timing logic generator. If two extra clock

drivers are used, care must be taken to ensure the rising and

falling edges of the H1BR and H2BR clocks occur at the

same time (within 3 ns) as the other HCCD clocks.

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Output

Figure 7. Output Architecture

VDD VOUT

Floating

Diffusion

HCCD

Charge

Transfer

Source

Follower

Source

Follower

Source

Follower

H2B

H1S

H1B

H2S

H2B

H1S

VDD

VSS

Charge packets contained in the horizontal register are

dumped pixel by pixel onto the floating diffusion (FD)

output node whose potential varies linearly with the quantity

of charge in each packet. The amount of potential charge is

determined by the expression DVFD =DQ/C

FD.

A three-stage source-follower amplifier is used to buffer

this signal voltage of f chip with slightly less than unity gain.

The translation from the charge domain to the voltage

domain is quantified by the output sensitivity or charge to

voltage conversion in terms of microvolts per electron

(mV/e−). After the signal has been sampled off chip, the reset

clock (R) removes the char ge from the floating dif fusion and

resets its potential to the reset drain voltage (RD).

When the image sensor is operated in the binned or

summed interlaced modes ther e w il l be mo re tha n 4 0, 000 e−

in the output signal. The image sensor is designed with

a16mV/e charge to voltage conversion on the output. This

means a full signal of 40,000 electrons will produce

a 640 mV change on the output amplifier. The output

amplifier was designed to handle an output swing of 640 mV

at a pixel rate of 40 MHz. If 80,000 electron charge packets

are generated in the binned or summed interlaced modes

then the output amplifier output will have to swing

1,280 mV. The output amplifier does not have enough

bandwidth (slew rate) to handle 1,280 mV at 40 MHz.

Hence, the pixel rate will have to be reduced to 20 MHz if

the full dynamic range of 80,000 electrons is desired.

The charge handling capacity of the output amplifier is

also set by the reset clock voltage levels. The reset clock

driver circuit is very simple if an amplitude of 5 V is used.

But the 5 V amplitude restricts the output amplifier charge

capacity to 40,000 electrons. If the full dynamic range of

80,000 electrons is desired then the reset clock amplitude

will have to be increased to 7 V.

If you only want a maximum signal of 40,000 electrons in

binned or summed interlaced modes, then a 40 MHz pixel

rate with a 5 V reset clock may be used. The output of the

amplifier will be unpredictable above 40,000 electrons so be

sure to set the maximum input signal level of your analog to

digital converter to the equivalent of 40,000 electrons

(640 mV).

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Pin Description and Physical Orientation

Figure 8. Package Pin Designations − Top View

Pixel 1,1

VSS

VOUTL

ESD

fV2

fV1

VSUB

GND

VDDL

VDDR

GND

VSUB

fV1

fV2

GND

VOUTR

VSS

fRL

fH2BL

fH1BL

fH1SL

fH2SL

GND

OGL

RDL

RDR

OGR

fFD

fH2SR

fH1SR

fH1BR

fH2BR

fRR

Pixel 1, 1

Table 4. PIN DESCRIPTION

Pin Name Description

1fRL Reset Gate, Left

2fH2BL H2 Barrier, Left

3fH1BL H1 Barrier, Left

4fH1SL H1 Storage, Left

5fH2SL H2 Storage, Left

6 GND Ground

7 OGL Output Gate, Left

8 RDL Reset Drain, Left

9 RDR Reset Drain, Right

10 ORG Output Gate, Right

11 FD Fast Line Dump Gate

12 fH2SR H2 Storage, Right

13 fH1SR H1 Storage, Right

14 fH1BR H1 Barrier, Right

15 fH2BR H2 Barrier, Right

16 fRR Reset Gate, Right

Pin Name Description

17 VSS Output Amplifier Return

18 VOUTR Video Output, Right

19 GND Ground

20 fV2 Vertical Clock, Phase 2

21 fV1 Vertical Clock, Phase 1

22 VSUB Substrate

23 GND Ground

24 VDDR VDD, Right

25 VDDL VDD, Left

26 GND Ground

27 VSUB Substrate

28 fV1 Vertical Clock, Phase 1

29 fV2 Vertical Clock, Phase 2

30 ESD ESD

31 VOUTL Video Output, Left

32 VSS Output Amplifier Return

NOTE: The pins are on a 0.070″ spacing.

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IMAGING PERFORMANCE

Table 5. TYPICAL OPERATIONAL CONDITIONS

(Unless otherwise noted, the Imaging Performance Specifications are measured using the following conditions.)

Description Condition Notes

Frame Time 237 ms 1

Horizontal Clock Frequency 10 MHz

Light Source Continuous Red, Green and Blue LED Illumination Centered at 450, 530 and 650 nm 2, 3

Operation Nominal Operating Voltages and Timing

1. Electronic shutter is not used. Integration time equals frame time.

2. LEDs used: Blue: Nichia NLPB500, Green: Nichia NSPG500S and Red: HP HLMP−8115.

3. For monochrome sensor, only green LED used.

Specifications

Table 6. PERFORMANCE SPECIFICATIONS

Description Symbol Min. Nom. Max. Unit Sampling

Plan

Temperature

Tested at

(5C)

ALL CONFIGURATIONS

Dark Center Uniformity N/A N/A 20 e− rms Die 27, 40

Dark Global Uniformity N/A N/A 5.0 mVpp Die 27, 40

Global Uniformity (Note 1) N/A 2.5 5.0 % rms Die 27, 40

Global Peak to Peak Uniformity

(Note 1) PRNU N/A 10 20 % pp Die 27, 40

Center Uniformity (Note 1) N/A 1.0 2.0 % rms Die 27, 40

Maximum Photoresponse

Non-Linearity (Notes 2, 3) NL N/A 2 − % Design

Maximum Gain Difference between

Outputs (Notes 2, 3) DGN/A 10 − % Design

Max. Signal Error due to Non-Linearity

Dif. (Notes 2, 3) DNL N/A 1 − % Design

Horizontal CCD Charge Capacity HNe N/A 100 N/A ke−Design

Vertical CCD Charge Capacity VNe N/A 50 N/A ke−Die

Photodiode Charge Capacity PNe 38 40 N/A ke−Die

Horizontal CCD Charge Transfer

Efficiency HCTE 0.99999 N/A N/A Design

Vertical CCD Charge Transfer

Efficiency VCTE 0.99999 N/A N/A Design

Photodiode Dark Current IPD N/A

N/A 40

0.01 350

0.1 e/p/s

nA/cm2Die 27, 40

Vertical CCD Dark Current IVD N/A

N/A 400

0.12 1,711

0.5 e/p/s

nA/cm2Die 27, 40

Image Lag Lag N/A < 10 50 e−Design

Anti-Blooming Factor XAB 100 300 N/A Design

Vertical Smear Smr N/A 80 75 dB Design

Total Noise (Note 4) ne−T − 23 − e− rms Design

Total Noise (Note 5) ne−T − 40 − e− rms Design

Dynamic Range (Notes 5, 6) DR − 60 − dB Design

Output Amplifier DC Offset VODC 4 8.5 14 V Die

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Table 6. PERFORMANCE SPECIFICATIONS (continued)

Description

Temperature

Tested at

(5C)

Sampling

Plan

UnitMax.Nom.Min.Symbol

ALL CONFIGURATIONS

Output Amplifier Bandwidth f−3DB − 140 − MHz Design

Output Amplifier Impedance ROUT 100 130 200 WDie

Output Amplifier Sensitivity DV/DN− 16 − mV/e−Design

KAI−2001−ABA CONFIGURATION

Peak Quantum Efficiency QEMAX 45 55 N/A % Design

Peak Quantum Efficiency Wavelength lQE N/A 500 N/A nm Design

KAI−2001−CBA CONFIGURATION

Peak Quantum Efficiency

Red

Green

Blue

QEMAX −

−

N/A

% Design

Peak Quantum Efficiency Wavelength

Red

Green

Blue

lQE −

−

620

540

470

N/A

nm Design

NOTE: N/A = Not Applicable.

1. Per color.

2. Value is over the range of 10% to 90% of photodiode saturation.

3. Value is for the sensor operated without binning.

4. Includes system electronics noise, dark pattern noise and dark current shot noise at 20 MHz.

5. Includes system electronics noise, dark pattern noise and dark current shot noise at 40 MHz.

6. Uses 20LOG (PNe /n

e−T).

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TYPICAL PERFORMANCE CUR VES

Quantum Efficiency

Monochrome with Microlens

Figure 9. Monochrome with Microlens Quantum Efficiency

0.0

0.1

0.2

0.3

0.4

0.5

0.6

400 500 600 700 800 900 1000

Wavelength (nm)

Absolute Quantum Efficiency

Measured with Glass

Monochrome without Microlens

Figure 10. Monochrome without Microlens Quantum Efficiency

0.00

0.02

0.04

0.06

0.08

0.10

0.12

240 340 440 540 640 740 840 940

Wavelength (nm)

Absolute Quantum Efficiency

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Color (Bayer RGB) with Microlens

Figure 11. Color (Bayer RGB) Quantum Efficiency

Wavelength (nm)

0.00

0.05

0.10

0.15

0.20

0.25

0.30

0.35

0.40

0.45

0.50

400 500 600 700 800 900 1000

Absolute Quantum Efficiency

Red

Green

Blue

Measured

with Glass

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Angular Quantum Efficiency

For the curves marked “Horizontal”, the incident light angle is varied in a plane parallel to the HCCD.

For the curves marked “Vertical”, the incident light angle is varied in a plane parallel to the VCCD.

Monochrome with Microlens

Figure 12. Angular Quantum Efficiency

Relative Quantum Efficiency (%)

Angle (degress)

100

0 5 10 15 20 25 30

Horizontal

Vertical

Dark Current vs. Temperature

Figure 13. Dark Current vs. Temperature

Electrons/Second

100

1,000

10,000

100,000

2.7 2.8 2.9 3.0 3.1 3.2 3.3 3.4

1000/T(K)

T (C) 97 84 72 60 50 40 30 21

VCCD

Photodiodes

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Power-Estimated

Figure 14. Power

Horizontal Clock Frequency (MHz)

Power (mW)

100

150

200

250

300

350

400

450

500

0 5 10 15 20 25 30 35 40

Right Output Disabled

Output Power One Output (mW)

Horizonatl Power (mW)

Vertical Power One Output (mW)

Total Power One Output (mW)

Frame Rates

Figure 15. Frame Rates

Pixel Clock (MHz)

Frame Rate (fps)

10 15 20 25 30 35 40

Dual 2×2 Binning

Dual Output or Single

2×2 Binning

Single Output

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DEFECT DEFINITIONS

Table 7. DEFECT DEFINITIONS

Description Definition Maximum Temperature(s)

Tested at (5C) Notes

Major Dark Field Defective Pixel Defect ≥ 179 mV 20 27, 40 1

Major Bright Field Defective Pixel Defect ≥ 15% 20 27, 40 1

Minor Dark Field Defective Pixel Defect ≥ 57 mV 200 27, 40

Cluster Defect A group of 2 to 10 contiguous major

defective pixels, but no more than 2 adjacent

defects horizontally.

827, 40 1

Column Defect A group of more than 10 contiguous major

defective pixels along a single column. 027, 40 1

1. There will be at least two non-defective pixels separating any two major defective pixels.

Defect Map

The defect map supplied with each sensor is based upon

testing at an ambient (27°C) temperature. Minor point defects are not included in the defect map. All defective

pixels are reference to pixel 1, 1 in the defect maps.

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TEST DEFINITIONS

Test Regions of Interest

Active Area ROI: Pixel (1, 1) to Pixel (1600, 1200)

Center 100 by 100 ROI: Pixel (750, 550) to

Pixel (849, 649)

Only the active pixels are used for performance and defect

tests.

Overclocking

The test system timing is configured such that the sensor

is overclocked in both the vertical and horizontal directions.

See Figure 16 for a pictorial representation of the regions.

Figure 16. Overclock Regions of Interest

Pixel 1,1

Vertical Overclock

Horizontal Overclock

Tests

Dark Field Center Non-Uniformity

This test is performed under dark field conditions. Only

the center 100 by 100 pixels of the sensor are used for this

test − pixel (750, 550) to pixel (849, 649).

Dark Field Center Uniformity +Standard Deviation of Center 100 by 100 Pixels in Electrons @ǒDPS Integration Time

Actual Integration Time UsedǓ

Units: mV rms. DPS Integration Time: Device Performance Specification Integration Time = 33 ms.

Dark Field Global Non-Uniformity

This test is performed under dark field conditions.

The sensor is partitioned into 192 sub regions of interest,

each of which is 100 by 100 pixels in size. See Figure 17.

The average signal level of each of the 192 sub regions of

interest is calculated. The signal level of each of the sub

regions of interest is calculated using the following formula:

Signal of ROI[i] +(ROI Average in ADU *

Units : mVpp (millivolts Peak to Peak)

*Horizontal Overclock Average in ADU) @

@mV per Count

Where i = 1 to 192. During this calculation on the 192 sub

regions of interest, the maximum and minimum signal levels

are found. The dark field global uniformity is then calculated

as the maximum signal found minus the minimum signal

level found.

Global Non-Uniformity

This test is performed with the imager illuminated to

a level such that the output is at 80% of saturation

(approximately 32,000 electrons). Prior to this test being

performed the substrate voltage has been set such that the

charge capacity of the sensor is 40,000 electrons. Global

uniformity is defined as:

Global Uniformi ty +100 @ǒActive Area Standard Deviation

Active Area Signal Ǔ

Active Area Signal = Active Area Average − H. Overclock Average

Units : % rms

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Global Peak to Peak Non-Uniformity

This test is performed with the imager illuminated to

a level such that the output is at 80% of saturation

(approximately 32,000 electrons). Prior to this test being

performed the substrate voltage has been set such that the

charge capacity of the sensor is 40,000 electrons. The sensor

is partitioned into 192 sub regions of interest, each of which

is 100 by 100 pixels in size. See Figure 17. The average

signal level of each of the 192 sub regions of interest (ROI)

is calculated. The signal level of each of the sub regions of

interest is calculated using the following formula:

Signal of ROI[i] +(ROI Average in ADU *

*Horizontal Overclock Average in ADU) @

@mV per Count

Where i = 1 to 192. During this calculation on the 192 sub

regions of interest, the maximum and minimum signal levels

are found. The global peak to peak uniformity is then

calculated as:

Global Uniformity +Max. Signal *Min. Signal

Active Area Signal

Units : % pp

Center Non-Uniformity

This test is performed with the imager illuminated to

a level such that the output is at 80% of saturation

(approximately 32,000 electrons). Prior to this test being

performed the substrate voltage has been set such that the

charge c a p a c ity of the sensor is 40,000 electrons. Defects are

excluded for the calculation of this test. This test is

performed on the center 100 by 100 pixels of the sensor (see

Figure 17). Center uniformity is defined as:

Center ROI Uniformity +100 @ǒCenter ROI Standard Deviation

Center ROI Signal Ǔ

Center ROI Signal = Center ROI Average − H. Overclock Average

Units : % rms

Dark Field Defect Test

This test is performed under dark field conditions.

The sensor is partitioned into 192 sub regions of interest,

each of which is 100 by 100 pixels in size (see Figure 17).

In each region of interest, the median value of all pixels is

found. For each region of interest, a pixel is marked

defective if it is greater than or equal to the median value of

that region of interest plus the defect threshold specified in

“Defect Definitions” section.

Bright Field Defect Test

This test is performed with the imager illuminated to

a level such that the output is at 80% of saturation

(approximately 32,000 electrons). Prior to this test being

performed the substrate voltage has been set such that the

charge capacity of the sensor is 40,000 electrons.

The average signal level of all active pixels is found.

The bright and dark thresholds are set as:

Dark Defect Threshold = Active Area Signal @Threshold

Bright Defect Threshold = Active Area Signal @Threshold

The sensor is then partitioned into 192 sub regions of

interest, each of which is 100 by 100 pixels in size (see

Figure 17). In each region of interest, the average value of

all pixels is found. For each region of interest, a pixel is

marked defective if it is greater than or equal to the median

value of that region of interest plus the bright threshold

specified or if it is less than or equal to the median value of

that region of interest minus the dark threshold specified.

Example for major bright field defective pixels:

•Average value of all active pixels is found to be

416 mV (32,000 electrons).

•Dark defect threshold: 416 mV ⋅ 15% = 62.4 mV.

•Bright defect threshold: 416 mV ⋅ 15% = 62.4 mV.

•Region of interest #1 selected. This region of interest is

pixels 1, 1 to pixels 100, 100.

♦Median of this region of interest is found to be

416 mV.

♦Any pixel in this region of interest that is

≥(416 + 62.4 mV) 478.4 mV in intensity will be

marked defective.

♦Any pixel in this region of interest that is

≥(416 − 62.4 mV) 353.6 mV in intensity will be

marked defective.

•All remaining 191 sub regions of interest are analyzed

for defective pixels in the same manner.

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Test Sub Regions of Interest

Figure 17. Test Sub Regions of Interest

Pixel

(1,1)

Pixel

(1600,1200

)

1 2 3 4 5 6 7 8 9 10

17 18 19 20 21 22 23 24 25 26

33 34 35 36 37 38 39 40 41 42

49 50 51 52 53 54 55 56 57 58

65 66 67 68 69 70 71 72 73 74

81 82 83 84 85 86 87 88 89 90

97 98 99 100 101 102 103 104 105 106

113 114 115 116 117 118 119 120 121 122

129 130 131 132 133 134 135 136 137 138

11 12 13 14 15 16

27 28 29 30 31 32

43 44 45 46 47 48

59 60 61 62 63 64

75 76 77 78 79 80

91 92 93 94 95 96

107 108 109 110 111 112

123 124 125 126 127 128

139 140 141 142 143 144

145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160

161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176

177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192

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OPERATION

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.

Table 8. ABSOLUTE MAXIMUM RATINGS

Description Symbol Minimum Maximum Unit Notes

Operating Temperature TOP −50 70 °C 1

Humidity RH 5 90 % 2

Output Bias Current IOUT 0.0 10 mA 3

Off-Chip Load CL− 10 pF 4

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 af fected.

1. Noise performance will degrade at higher temperatures.

2. T = 25°C. Excessive humidity will degrade MTTF.

3. Total for both outputs. Current is 5 mA for each output. Note that the current bias affects the amplifier bandwidth.

4. With total output load capacitance of CL = 10 pF between the outputs and AC ground.

Table 9. MAXIMUM VOLTAGE RATINGS BETWEEN PINS

Description Minimum Maximum Unit Notes

RL, RR, H1S, H2S, H1BL, H2BL, H1BR, H2BR, H1BR,

OGL, OGR to ESD 0 17 V

Pin to Pin with ESD Protection −17 17 V 1

VDDL, VDDR to GND 0 25 V

1. Pins with ESD protection are: RL, RR, H1S, H2S, H1BL, H2BL, H1BR, H2BR, OGL, and OGR.

Table 10. DC BIAS OPERATING CONDITIONS

Description Symbol Min. Nom. Max. Unit Maximum

DC Current Notes

Output Gate OG −3.0 −2.5 −2.0 V1 mA

Reset Drain RD 11.5 12.0 12.5 V 1 mA

Output Amplifier Supply VDD 14.5 15.0 15.5 V 1 mA 1

Ground GND 0.0 0.0 0.0 V

Substrate SUB 8.0 VAB 17.0 V 2, 4

ESD Protection ESD −8.0 −7.0 −6.0 V 3

Output Amplifier Return VSS 0.0 0.7 1.0 V

1. The operating value of the substrate voltage, V AB, will be marked on the shipping container for each device. The value VAB is set such that

the photodiode charge capacity is 40,000 electrons.

2. VESD must be at least 1 V more negative than H1L, H2L and RL during sensors operation AND during camera power turn on.

3. One output, unloaded.

4. Refer to Application Note Using Interline CCD Image Sensors in High Intensity Visible Lighting Conditions.

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AC Operating Conditions

Table 11. CLOCK LEVELS

Description Symbol Min. Nom. Max. Unit Notes

Vertical CCD Clock High V2H 7.5 8.0 8.5 V

Vertical CCD Clocks Midlevel V1M, V2M −0.2 0.0 0.2 V

Vertical CCD Clocks Low V1L, V2L −9.5 −9.0 −8.5 V

Horizontal CCD Clocks Amplitude H1H, H2H 4.5 5.0 5.5 V

Horizontal CCD Clocks Low H1L, H2L −5.0 −4.0 −3.8 V

Reset Clock Amplitude RH − 5.0 − V 1

Reset Clock Low RL −4.0 −3.5 −3.0 V 2

Electronic Shutter Voltage VSHUTTER 44 48 52 V 3

Fast Dump High FDH 4.8 5.0 5.2 V

Fast Dump Low FDL −9.5 −9.0 −8.0 V

1. Reset amplitude must be set to 7.0 V for 80,000 electrons output in summed interlaced or binning modes.

2. Reset low level must be set to –5.0 V for 80,000 electrons output in summed interlaced or binning modes.

3. Refer to Application Note Using Interline CCD Image Sensors in High Intensity Visible Lighting Conditions.

Clock Line Capacitances

Figure 18. Clock Line Capacitances

GND

25 nF

H1SL+H1BL 66 pF

H2SL+H2BL 58 pF

H1SR+H1BR 66 pF

H2SR+H2BR 58 pF

20 pF

GND

Reset

10 pF

GND

SUB

2 nF

GND

21 pF

5 nF

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TIMING

Table 12. TIMING REQUIREMENTS

Description Symbol Min. Nom. Max. Unit

HCCD Delay tHD 1.3 1.5 10.0 ms

VCCD Transfer Time tVCCD 1.3 1.5 20.0 ms

Photodiode Transfer Time tV3rd 8.0 12.0 15.0 ms

VCCD Pedestal Time t3P 20.0 25.0 50.0 ms

VCCD Delay t3D 15.0 20.0 100.0 ms

Reset Pulse Time tR5.0 10.0 − ns

Shutter Pulse Time tS3.0 5.0 10.0 ms

Shutter Pulse Delay tSD 1.0 1.6 10.0 ms

HCCD Clock Period tH25.0 50.0 200.0 ns

VCCD Rise/Fall Time tVR 0.0 0.1 1.0 ms

Fast Dump Gate Delay tFD 0.0 0.0 0.5 ms

Vertical Clock Edge Alignment tVE 0.0 − 100.0 ns

Timing Modes

Progressive Scan

Figure 19. Progressive Scan Operation

Photodiode CCD Shift Register

Output

HCCD

In progressive scan read out every pixel in the image

sensor is read out simultaneously. Each charge packet is

transferred from the photodiode to the neighboring vertical

CCD shift register simultaneously. The maximum useful

signal output is limited by the photodiode charge capacity to

40,000 electrons.

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Figure 20. Progressive Scan Flow Chart

Vertical Frame

Timing

Line Timing

Repeat for 1214

Lines

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Frame Timing

Frame Timing without Binning − Progressive Scan

Figure 21. Frame Timing without Binning

Line 1214 Line 1

t3D

t3P

tV3rd

Line 1213

Frame Timing for Vertical Binning by 2 − Progressive Scan

Figure 22. Frame Timing for Vertical Binning by 2

t3D

t3P

tV3rd

Line 607 Line 1

Line 606

3 × tVCCD

Frame Timing Edge Alignment

Figure 23. Frame Timing Edge Alignment

V1M

V1L

V2H

V2M

V2L

tVE

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Line Timing

Line Timing Single Output − Progressive Scan

Figure 24. Line Timing Single Output

Pixel Count

tVCCD

tHD

1625

1626

1627

1629

1630

1643

1644

1628

1642

Line Timing Dual Output − Progressive Scan

Figure 25. Line Timing Dual Output

Pixel Count

tVCCD

tHD

816

817

818

820

821

824

825

819

823

822

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Line Timing Vertical Binning by 2 − Pr ogressive Scan

Figure 26. Line Timing Vertical Binning by 2

Pixel Count

3 × tVCCD

tHD

1625

1626

1627

1629

1630

1643

1644

1628

1642

Line Timing Detail − Pr ogressive Scan

Figure 27. Line Timing Detail

tVCCD

tHD

1/2 tH

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Line Timing Binning by 2 Detail − Progressive Scan

Figure 28. Line Timing Binning by 2 Detail

tVCCD tHD

1/2 tHtVCCD tVCCD

Line Timing Edge Alignment

Figure 29. Line Timing Edge Alignment

tVE

VCCD

tVE

NOTE: Applies to all modes.

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Pixel Timing

Figure 30. Pixel Timing

Dummy Pixels Light Shielded Pixels Photosensitive Pixels

VOUT

Pixel

Count

19 20 21

Pixel Timing Detail

Figure 31. Pixel Timing Detail

VOUT

H1H

H1L

H2H

H2L

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Fast Line Dump Timing

Figure 32. Fast Line Dump Timing

tFD

tVCCD

tFD tVCCD

fFD

fV1

fV2

fH2

fH1

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Electronic Shutter

Electronic Shutter Line Timing

Figure 33. Electronic Shutter Line Timing

tHD

tVCCD

VSUB

fV1

fV2

fH2

fH1

tSD

VSHUTTER

Electronic Shutter − Integration Time Definition

Figure 34. Integration Time Definition

VSUB

fV2

VSHUTTER

Integration Time

Electronic Shutter − DC and AC Bias Definition

The figure below shows the DC bias (VSUB) and AC clock (VES) applied to the SUB pin. Both the DC bias and AC clock

are referenced to ground.

Figure 35. DC Bias and AC Clock Applied to the SUB Pin

SUB

GND GND

SHUTTER

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Electronic Shutter Description

The voltage on the substrate (SUB) determines the charge

capacity of the photodiodes. When SUB is 8 V the

photodiodes will be at their maximum charge capacity.

Increasing VSUB above 8 V decreases the charge capacity

of the photodiodes until 48 V when the photodiodes have

a charge capacity of zero electrons. Therefore, a short pulse

on SUB, with a peak amplitude greater than 48 V, empties

all photodiodes and provides the electronic shuttering

action.

It may appear the optimal substrate voltage setting is 8 V

to obtain the maximum charge capacity and dynamic range.

While setting VSUB to 8 V will provide the maximum

dynamic range, it will also provide the minimum

anti-blooming protection.

The KAI−2001 VCCD has a charge capacity of

55,000 electrons ( 5 5 ke−). If the SUB voltage is set such that

the photodiode holds more than 55 ke−, then when the

charge is transferred from a full photodiode to VCCD,

the VCCD will overflow. This overflow condition manifests

itself in the image by making bright spots appear elongated

in the vertical direction. The size increase of a bright spot is

called blooming when the spot doubles in size.

The blooming can be eliminated by increasing the voltage

on SUB to lower the charge capacity of the photodiode. This

ensures the VCCD charge capacity is greater than the

photodiode capacity. There are cases where an extremely

bright spot will still cause blooming in the VCCD. Normally,

when the photodiode is full, any additional electrons

generated by photons will spill out of the photodiode.

The excess electrons are drained harmlessly out to the

substrate. There is a maximum rate at which the electrons

can be drained to the substrate. If that maximum rate is

exceeded, (for example, by a very bright light source) then

it is possible for the total amount of charge in the photodiode

to exceed the VCCD capacity. This results in blooming.

The amount of anti-blooming protection also decreases

when the integration time is decreased. There is

a compromise between photodiode dynamic range

(controlled by VSUB) and the amount of anti-blooming

protection. A low VSUB voltage provides the maximum

dynamic range and minimum (or no) anti-blooming

protection. A high VSUB voltage provides lower dynamic

range and maximum anti-blooming protection. The optimal

setting of VSUB is written on the container in which each

KAI−2001 is shipped. The given VSUB voltage for each

sensor is selected to provide anti-blooming protection for

bright spots at least 100 times saturation, while maintaining

at least 40 ke− of dynamic range.

The electronic shutter provides a method of precisely

controlling the image exposure time without any

mechanical components. If an integration time of tINT is

desired, then the substrate voltage of the sensor is pulsed to

at least 40 V tINT seconds before the photodiode to VCCD

transfer pulse on V2. Use of the electronic shutter does not

have to wait until the previously acquired image has been

completely read out of the VCCD.

Large Signal Output

When the image sensor is operated in the binned or

summed interlaced modes there will be more than

40,000 electrons in the output signal. The image sensor is

designed with a 16 mV/e charge to voltage conversion on the

output. This means a full signal of 40,000 electrons will

produce a 640 mV change on the output amplifier.

The output amplifier was designed to handle an output

swing of 640 mV at a pixel rate of 40 MHz. If 80,000

electron charge packets are generated in the binned or

summed interlaced modes then the output amplifier output

will have to swing 1,280 mV. The output amplifier does not

have enough bandwidth (slew rate) to handle 1,280 mV at

40 MHz. Hence, the pixel rate will have to be reduced to

20 MHz if the full dynamic range of 80,000 electrons is

desired.

The charge handling capacity of the output amplifier is

also set by the reset clock voltage levels. The reset clock

driver circuit is very simple if an amplitude of 5 V is used.

But the 5 V amplitude restricts the output amplifier charge

capacity to 40,000 electrons. If the full dynamic range of

80,000 electrons is desired then the reset clock amplitude

will have to be increased to 7 V.

If you only want a maximum signal of 40,000 electrons in

binned or summed interlaced modes, then a 40 MHz pixel

rate with a 5 V reset clock may be used. The output of the

amplifier will be unpredictable above 40,000 electrons so be

sure to set the maximum input signal level of your analog to

digital converter to the equivalent of 40,000 electrons

(640 mV).

KAI−2001

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STORAGE AND HANDLING

Table 13. STORAGE CONDITIONS

Description Symbol Minimum Maximum Unit Notes

Storage Temperature TST −55 80 °C 1

Humidity RH 5 90 % 2

1. Long-term exposure toward the maximum temperature will accelerate color filter degradation.

2. T = 25°C. Excessive humidity will degrade 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 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 soldering recommendations, please

download the Soldering and Mounting Techniques

Reference Manual (SOLDERRM/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 Standard terms and Conditions of

Sale, please download Terms and Conditions from

www.onsemi.com.

KAI−2001

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MECHANICAL DRAWINGS

Completed Assembly

Figure 36. Completed Assembly

1. See Ordering Table for marking code.

2. Cover glass is manually placed and visually aligned

over die − Location accuracy is not guaranteed.

Notes:

Dimensions Units: IN [MM]

Tolerances: Unless otherwise specified

Ceramic ±1% no less than 0.005″

L/F ±1% no more than 0.005″

KAI−2001

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Die to Package Alignment

Figure 37. Die to Package Alignment

1. Center of image is offset from center of package

by (0.00, 0.00) mm nominal.

2. Die is aligned within ±2 degree of any package

cavity edge.

Notes:

Dimensions Units: IN [MM]

Tolerances: Unless otherwise specified

Ceramic ±1% no less than 0.005″

L/F ±1% no more than 0.005″

KAI−2001

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Glass

Figure 38. Glass Drawing

1. Materials: Substrate − Schott D236T eco or equivalent

Epoxy: NCO−150HB

Thickness: 0.002″−0.005″

2. Dust, Scratch Count − 10 microns max.

3. Reflectance:

420−435 nm < 2%

435−630 nm < 0.8%

630−680 nm < 2%

Notes:

Units: IN [MM]

Tolerance: Unless otherwise specified

±1% no less than 0.005″

Double Sided AR Coated Glass

1. Materials: Substrate − Schott D236T eco or equivalent

2. No Epoxy

3. Dust, Scratch Count − 10 microns max.

4. Reflectance:

420−435 nm < 10%

435−630 nm < 10%

630−680 nm < 10%

Clear Glass

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Glass Transmission

Figure 39. Glass Transmission

100

200 300 400 500 600 700 800 900

Wavelength (nm)

Transmission (%)

Clear

MAR

Figure 40. Quartz Glass Transmission

100

200 300 400 500 600 700 800 900

Wavelength (nm)

Transmission (%)

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specifically disclaims any and all l iabilit y, including without limitation special, consequential or i ncident al d amages. “Typical” parameters which may be pr ovided i n 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

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USA/Canada

Europe, Middle East and Africa Technical Support:

Phone: 421 33 790 2910

Japan Customer Focus Center

Phone: 81−3−5817−1050

KAI−2001/D

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Fax: 303−675−2176 or 800−344−3867 Toll Free USA/Canada

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