cxa3796n camera

3
Expanded input dynamic range Low-noise/high-gain AGC amplifier Supports switching of the AGC amplifier maximum gain and negative gain Blanking function CDS clamp function Sample-and-hold and reference voltage output functions other factors, the CXA3796N can continuously match this DC level to a reference voltage black level using the externally provided CLPDM signal. This makes it possible to always maintain a fixed black level even under different usage conditions. Since an A/D converter is connected to the CXA3796N in the following stages, the CXA3796N output includes a sample-and- hold function that is applied to each pixel. This reduces problems such as signal degradation due to inadequate settling. Photograph 1 shows an example of imaging using this device. Excellent images can be obtained even under low illumination due to the reduced noise. and can directly replace that device with no changes. (The MAXGAIN and GAINSHIFT pins correspond to NC and PS (Power Save) pins in the CXA2096N, and operate in CXA2096N mode when the CXA3796N replaces the CXA2096N with no changes to the application circuit.) Any of nine gain curves can be selected by the voltages applied to the MAXGAIN and GAINSHIFT pins. (See table 1 and figure 2.) Since the CXA3796N is designed in particular to also handle negative gains, it can provide a long-desired and effective solution to the color rolling phenomenon. The AGC amplifier circuit structure was revised in the CXA3796N to achieve noise reduction. The inclusion of a blanking function that disables the CCDLEVEL output during blanking also contributes to reduced noise. Figure 3 shows the gain and output noise characteristics. When compared at the same 26 dB gain, the CXA3796N provides a noise reduction effect of 4 to 5 dB. (Note: This value differs depending on the camera system.) While the CCD pixel outputs have large differences in the DC levels due to temperature, sample-to-sample variations, and CCD Camera Head Amplifier  with High-Gain/Low-Noise Amplifier There are increasing needs for security cameras that support nighttime imaging. Sony has now developed the CXA3796N CCD camera head amplifier that is optimal for this sort of low- illumination imaging. This new product is pin compatible with the existing CXA2096N, and now allows the maximum gain and the negative g ain to be s et externall y. By achieving even lower noise than the CXA2096N, the CXA3796N allows Sony to provide an optimal solution not only for CXA2096N users, but for all users concerned with low-illumination imaging. CXA3796N This IC is a CCD security camera head amplifier. Security cameras are requred to produce bright and clear images even in dark places and at dark times of day. To respond to those needs, we achieved even higher gain and lower noise characteristics than in existi ng products. In the low-no ise design, it was particularly important to suppress noise in the signal lines from the input to the AGC, and all the members of the development team worked together as a group on the low-noise design for the S/H and AGC circuits. I strongly recommend that you consider this product. The CXA3796N is a bipolar IC that was developed as a CCD camera head amplifier appropriate for low-illumination imaging with security cameras and similar products. After applying noise exclusion by correlated double sampling (CDS) to the pixel output signals from the CCD, the signals are amplified with an automatic gain control (AGC) amplifier and output to the A/D converter in the DSP in the later stages of the system. The block diagram of the CXA3796N includes the CDS circuit, the AGC amplifier for the CCD output signal, a camera sample-and-hold (S/H) circuit for the external A/D converter, A/D converter reference voltage output circuits, and a CCDLEVEL output circuit for monitoring. (See figure 1.) The CXA3796N is pin compatible with the existing CXA2096N, Pin Compatibility with the Existing CXA2096N Low-Illumination Imaging Nine Gain Curves Noise Reduced by 4 to 5 dB Black Level Set by CDS Clamping

Upload: shikhar623

Post on 14-Apr-2018

215 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: cxa3796n Camera

7/27/2019 cxa3796n Camera

http://slidepdf.com/reader/full/cxa3796n-camera 1/2

■ Expanded input dynamic range

■ Low-noise/high-gain AGC amplifier

■ Supports switching of the AGCamplifier maximum gain andnegative gain

■ Blanking function

■ CDS clamp function

■ Sample-and-hold and referencevoltage output functions

other factors, the CXA3796N can continuously

match this DC level to a reference voltageblack level using the externally provided

CLPDM signal. This makes it possible to

always maintain a fixed black level even under

different usage conditions.

Since an A/D converter is connected to the

CXA3796N in the following stages, the

CXA3796N output includes a sample-and-

hold function that is applied to each pixel.

This reduces problems such as signal

degradation due to inadequate settling.

Photograph 1 shows an example of imagingusing this device. Excellent images can be

obtained even under low illumination due to

the reduced noise.

and can directly replace that device with no

changes. (The MAXGAIN and GAINSHIFTpins correspond to NC and PS (Power Save)

pins in the CXA2096N, and operate in

CXA2096N mode when the CXA3796N

replaces the CXA2096N with no changes to

the application circuit.)

Any of nine gain curves can be selected by the

voltages applied to the MAXGAIN and

GAINSHIFT pins. (See table 1 and figure 2.)

Since the CXA3796N is designed in particular

to also handle negative gains, it can provide a

long-desired and effective solution to the colorrolling phenomenon.

The AGC amplifier circuit structure was

revised in the CXA3796N to achieve noise

reduction. The inclusion of a blanking function

that disables the CCDLEVEL output during

blanking also contributes to reduced noise.

Figure 3 shows the gain and output noise

characteristics. When compared at the same 26

dB gain, the CXA3796N provides a noise

reduction effect of 4 to 5 dB. (Note: This value

differs depending on the camera system.)

While the CCD pixel outputs have large

differences in the DC levels due to

temperature, sample-to-sample variations, and

CCD Camera Head Amplifier with High-Gain/Low-Noise Amplifier

There are increasing needs for security cameras that support nighttime imaging.

Sony has now developed the CXA3796N CCD camera head amplifier that is optimal for this sort of low-

illumination imaging.

This new product is pin compatible with the existing CXA2096N, and now allows the maximum gain and the

negative gain to be set externally.

By achieving even lower noise than the CXA2096N, the CXA3796N allows Sony to provide an optimal

solution not only for CXA2096N users, but for all users concerned with low-illumination imaging.

CXA3796N

This IC is a CCD security camera head

amplifier. Security cameras are requred to

produce bright and clear images even indark places and at dark times of day. To

respond to those needs, we achieved even

higher gain and lower noise characteristicsthan in existing products. In the low-noise

design, it was particularly important to

suppress noise in the signal lines from theinput to the AGC, and all the members of

the development team worked together asa group on the low-noise design for the

S/H and AGC circuits. I strongly

recommend that you consider this product.

The CXA3796N is a bipolar IC that was

developed as a CCD camera head amplifier

appropriate for low-illumination imaging with

security cameras and similar products. After

applying noise exclusion by correlated double

sampling (CDS) to the pixel output signals

from the CCD, the signals are amplified with

an automatic gain control (AGC) amplifier

and output to the A/D converter in the DSP in

the later stages of the system.

The block diagram of the CXA3796N includes

the CDS circuit, the AGC amplifier for the

CCD output signal, a camera sample-and-hold(S/H) circuit for the external A/D converter,

A/D converter reference voltage output circuits,

and a CCDLEVEL output circuit for

monitoring. (See figure 1.) The CXA3796N

is pin compatible with the existing CXA2096N,

Pin Compatibilitywith the Existing CXA2096N

Low-Illumination Imaging

Nine Gain Curves

Noise Reduced by 4 to 5 dB

Black Level Set by CDS Clamping

Page 2: cxa3796n Camera

7/27/2019 cxa3796n Camera

http://slidepdf.com/reader/full/cxa3796n-camera 2/2

Correlated double

sampling (CDS)

+

 – 

Automatic gain

control (AGC)

CDS clamp

Camera

S/H

Output

buffer

Output

buffer

PIN

DIN

CCDLEVEL

DRVOUT

VRB

VRT

VIN

VRB

EVR

VRT

A/Dconverter

   A   G   C   C   O   N   T

   M   A   X   G   A   I   N

   O   P   E   N

   G   N   D

   V   C   C

   G   A   I   N   S   H   I   F   T

DSP

CXA3796N

VOUTCCD

   O   P   E   N

   G   N   D

   V   C   C

GAINSHIFT = VCC (0 dB)

 –5

0

5

10

15

20

25

30

35

40

0.5 0.6 0.7 0.8 0.9 1

VAGCCONT / VCC

   G  a   i  n   [   d   B   ]

MAXGAIN = VCC (34 dB mode)

MAXGAIN = GND (30 dB mode)

MAXGAIN = OPEN (26 dB mode)

0

0.5

1

1.5

2

2.5

3

3.5

4

4.5

5

0 5 10 15 20 25 30 35

Gain [dB]

   O  u   t  p  u   t  n

  o   i  s  e   [  m   V  r  m  s   ]

CXA3796N

CXA2096N

MAXGAIN GAINSHIFT Gain

VCC 0 dB to 34 dB

OPEN –3 dB to 31 dBVCC

GND  –6 dB to 28 dB

VCC 0 dB to 30 dB

OPEN –3 dB to 27 dBGND

GND  –6 dB to 24 dB

VCC 0 dB to 26 dB

OPEN  –3 dB to 23 dBOPEN

GND  –6 dB to 20 dB

CXA3796N (1000lx, F5.6, 1/60 s, 34 dB mode)

Block DiagramFigure 1

Gain vs. Output NoiseFigure 3Gain Curves (when GAINSHIFT = VCC)Figure 2

Imaging ExamplePhotograph 1 MAXGAIN and GAINSHIFT SettingsTable 1