MT9V124EBKSTCD-GEVK - Aptina

June, 2018 − Rev. 6

1Publication Order Number:

MT9V124/D

MT9V124

MT9V124 1/13‐Inch

System‐On‐A‐Chip (SOC)

CMOS Digital Image Sensor

GENERAL DESCRIPTION

ON Semiconductor’s MT9V124 is a 1/13-inch CMOS digital image

sensor with an active-pixel array of 648 (H) × 488 (V). It includes

sophisticated camera functions such as auto exposure control, auto

white balance, black level control, flicker detection and avoidance,

and defect correction. It is designed for low light performance. It is

programmable through a simple two-wire serial interface. The

MT9V124 produces extraordinarily clear, sharp digital pictures that

make it the perfect choice for a wide range of medical and industrial

applications.

Table 1. KEY PARAMETERS

Parameter Typical Value

Optical Format 1/13-inch

Active Pixels 648 × 488 = 0.3 Mp (VGA)

Pixel Size 1.75 μm

Color Filter Array RGB Bayer

Shutter Type Electronic Rolling Shutter (ERS)

Input Clock Range 18–44 MHz

Output LVDS 12-bit Packet

Frame Rate, Full Resolution 30 fps

Responsivity 1.65 V/lux ×sec

SNRMAX 33.4 dB

Dynamic Range 58 dB

Supply Voltage

Analog 2.5–3.1 V

Digital 1.7–1.95 V

Digital I/O 1.7–1.95 V or 2.5–3.1 V

Power Consumption 55 mW

Operating Temperature (Ambient) −TA–30°C to +70°C

Chief Ray Angle 24°

Package Options Bare die, CSP

Features

•Superior Low-light Performance

•Ultra-low-power

•VGA Video at 30fps

•Internal Master Clock Generated by On-chip Phase Locked Loop

(PLL) Oscillator

•Electronic Rolling Shutter (ERS), Progressive Scan

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See detailed ordering and shipping information on page 2 of

this data sheet.

ORDERING INFORMATION

ODCSP25 2.694 × 2.694

CASE 570BN

Features (continued)

•Integrated Image Flow Processor (IFP) for

Single-die Camera Module

•One-time Programmable Memory (OTPM)

•Automatic Image Correction and

Enhancement, Including Four-channel Lens

Shading Correction

•Image Scaling with Anti-aliasing

•Supports ITU-R BT.656 Format with Odd

Timing Code

•Two-wire Serial Interface Providing Access

to Registers and Microcontroller Memory

•Selectable Output Data Format: YCbCr,

565RGB, and RAW8+2-bit, BT656

•High Speed Serial Data Output in 12-bit

Packet

•Independently Configurable Gamma

Correction

•Direct XDMA Access

(Reducing Serial Commands)

•Integrated Hue Rotation ±22°

Applications

•Medical Tools, Device

•Biometrics

•Industrial Application

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ORDERING INFORMATION

Table 2. AVAILABLE PART NUMBERS

Part Number Product Description Orderable Product Attribute Description †

MT9V124D00STCK22DC1−200 RGB color die Die Sales, 200 μm Thickness

MT9V124EBKSTC−CR CSP with 400 μm coverglass Chip Tray without Protective Film

†For information on tape and reel specifications, including part orientation and tape sizes, please refer to our Tape and Reel Packaging

Specification Brochure, BRD8011/D.

FUNCTIONAL DESCRIPTION

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.

ON Semiconductor’s MT9V124 is a 1/13-inch VGA

CMOS digital image sensor with an integrated advanced

camera system. This camera system features a

microcontroller (MCU), a sophisticated image flow

processor (IFP), and a serial port (using LVDS signaling).

The microcontroller manages all functions of the camera

system and sets key operation parameters for the sensor core

to optimize the quality of raw image data entering the IFP.

The sensor core consists of an active pixel array of

648 ×488 pixels with programmable timing and control

circuitry. It also includes an analog signal chain with

automatic offset correction, programmable gain, and a

10-bit analog-to-digital converter (ADC).

The entire system-on-a-chip (SOC) has an ultra-low

power operational mode and a superior low-light

performance that is particularly suitable for medical

applications. The MT9V124 features ON Semiconductor’s

breakthrough low-noise CMOS imaging technology that

achieves near-CCD image quality (based on signal-to-noise

ratio and low-light sensitivity) while maintaining the

inherent size, cost, and integration advantages of CMOS.

Architecture Overview

The MT9V124 combines a VGA sensor core with an IFP

to form a stand-alone solution for both image acquisition

and processing. Both the sensor core and the IFP have

internal registers that can be controlled by the user. In

normal operation, an integrated microcontroller

autonomously controls most aspects of operation. The

processed image data is transmitted to the external host

system through an LVDS bus. Figure 1 shows the major

functional blocks of the MT9V124.

Figure 1. MT9V124 Block Diagram

F IFO

STANDBY

EXTCLK

Analog

Processing ADC Digital Image

Processing (SOC)

PLL

Pixel Array

(648 x 488)

Column Control

RAM ROM

uControroller

CCI Serial

Interface SDATA

SCLOCK

Column Control

VDD

VDDIO

VPP

VAA

Image Data Bus

Serializer

LVDS_N

LVDS_P

AGND DGND

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Sensor Core

The MT9V124 has a color image sensor with a Bayer

color filter arrangement and a VGA active-pixel array with

electronic rolling shutter (ERS). The sensor core readout is

10 bits. The sensor core also supports separate analog and

digital gain for all four color channels (R, Gr, Gb, B).

Image Flow Processor (IFP)

The advanced IFP features and flexible programmability

of the MT9V124 can enhance and optimize the image sensor

performance. Built-in optimization algorithms enable the

MT9V124 to operate with factory settings as a fully

automatic and highly adaptable system-on-a-chip (SOC) for

most camera systems.

These algorithms include shading correction, defect

correction, color interpolation, edge detection, color

correction, aperture correction, and image formatting with

cropping and scaling.

Microcontroller Unit (MCU)

The MCU communicates with all functional blocks by

way of an internal ON Semiconductor proprietary bus

interface. The MCU firmware executes the automatic

control algorithms for exposure and white balance.

System Control

The MT9V124 has a phase-locked loop (PLL) oscillator

that can generate the internal sensor clock from the common

system clock. The PLL adjusts the incoming clock

frequency up, allowing the MT9V124 to run at almost any

desired resolution and frame rate within the sensor’s

capabilities.

Low-power consumption is a very important requirement

for all components of wireless devices. The MT9V124

provides power-conserving features, including an internal

soft standby mode and a hard standby mode.

A two-wire serial interface bus enables read and write

access to the MT9V124’s internal registers and variables.

The internal registers control the sensor core, the color

pipeline flow, the output interface, auto white balance

(AWB) and auto exposure (AE).

Output Interface

The output interface block can select either raw data or

processed data. Image data is provided to the host system by

an LVDS serial interface. The LVDS output port provides

8-bit YCbCr, YUV, 565 RGB, BT656, processed Bayer data

or extended 10-bit Bayer data achieved using 8 + 2 format.

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System Interfaces

Figure 2 shows typical MT9V124 device connections.

For low-noise operation, the MT9V124 requires separate

power supplies for analog and digital sections. Both power

supply rails should be decoupled from ground using

capacitors as close as possible to the die.

The MT9V124 provides dedicated signals for digital core

and I/O power domains that can be at different voltages. The

PLL and analog circuitry require clean power sources.

Table 3, “Pin Descriptions,” provides the signal descriptions

for the MT9V124.

Figure 2. Typical Configuration (Connection)

Notes:

VDD_IO3, 4

Analog

power

SDATA

SCLK

LVDS_P

STANDBY

AGND

Two−wire

serial interface

Serial

interface

Active HIGH standby mode

EXTCLK

External clock in

(18–44 MHz)

GND, GND_PLL

LVDS_N

VDD4VAA4

140 Ω

RPULL−UP2

I/O3

Power

OTPM

Power

(optimal)

Digital

Core

(optimal)

VDD_IO

VPP

VDD

VAA

1. This typical configuration shows only one scenario out of multiple possible variations for this sensor.

2. ON Semiconductor recommends a 1.5 kΩ resistor value for the two-wire serial interface RPULL-UP; however, greater

values may be used for slower transmission speed.

3. All inputs must be configured with VDD_IO.

4. ON Semiconductor recommends that 0.1 μF and 1 μF decoupling capacitors for each power supply are mounted as

close as possible to the module (Low-Z path). Actual values and numbers may vary depending on layout and design

considerations, such as capacitor effective series resistance (ESR), dielectric, or power supply source impedance.

5. LVDS output requires termination resistor (140 Ω) to be placed closely at the sensor side.

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Signal Descriptions

Table 3. PIN DESCRIPTIONS

MT9V124

Sensor Signal

Name

Module Signal

Name Ball Number Type Description

EXTCLK EXTCLK E2 Input Input clock signal

STANDBY STBY A2 Input Controls sensor’s standby mode, active HIGH

SCLK SCLK D4 Input Two-wire serial interface clock

SDATA SDATA E4 I/O Two-wire serial interface data

LVDS_P LVDS_P E1 Output LVDS positive output

LVDS_N LVDS_N D2 Output LVDS negative output

VDD VDD C2, D5 Supply Digital power (TYP 1.8 V)

VAA, VDD_PLL VAA C1 Supply Analog and PLL power (TYP 2.8 V)

VDD_IO VDD_IO C3 Supply I/O power supply (TYP 1.8 V)

DGND, GND_IO,

GND_PLL

DGND B3, B5, D1 Supply Digital, I/O, and PLL ground

AGND AGND B1 Supply Analog ground

VPP VPP A1 Supply OTPM power

DNU DNU A3,A4,A5,B2,B4,

C4,C5,D3,E3,E5

Figure 3. 25-ball Assignments (Top View)

VPP DNU

VAA

GND

DNU

VDD

DNUSTDBY

VDD_IO

DNU

AGND

SDATA

DNU DNU

EXTCLK

LVDS_P

DNU SCLK

DNU

GND GND

DNU

LVDS_N

VDD

123 4 5

Power-On Reset

The MT9V124 includes a power-on reset feature that

initiates a reset upon power-up. A soft reset is issued by

writing commands through the two-wire serial interface.

Standby

The MT9V124 supports two different standby modes:

•Hard standby mode

•Soft standby mode

The hard standby mode is invoked by asserting

STANDBY pin. It then disables all the digital logic within

the image sensor, and only supports being awoken by

de-asserting the STANDBY pin. The soft standby mode is

enabled by a single register access, which then disables the

sensor core and most of the digital logic. However, the

two-wire serial interface is kept alive, which allows the

image sensor to be awoken via a serial register access.

All output signal status during standby are shown in

Table 4.

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Table 4. Status of Output Signals During Reset and Standby

Signal Reset Post-Reset Standby

LVDS_P High−ZHigh−ZHigh−Z

LVDS_N High−ZHigh−ZHigh−Z

Module ID

The MT9V124 provides 4 bits of module ID that can be

read by the host processor from register 0x001A[15:12].

The module ID is programmed through the OTPM.

Image Data Output Interface

The High Speed LVDS output port on MT9V124 can

transmit the sensor image data to the host system over a

lengthy differential twisted pair cable.

The MT9V124 provides a serial high-speed output port,

which is able for driving standard IEEE 1596.3−1996 LVDS

receiver/deserializers such as the DS92LV1212A LVDS

Deserializer by National Semiconductor.

Image data is provided to the host system by the serial

LVDS interface. The Start bit, 8-bit image data, LV, FV, and

Stop bit are packetized in a 12-bit packet. The output

interface block can select either raw data or processed data.

Processed data format includes YCbCr, RGB-565, and

BT656 with odd SAV/EAV code. It also supports the SOC

Bypass 8 + 2 data format over the 12-bit packet.

The LVDS port is disabled when Hard Standby or Soft

Standby is asserted.

Sensor Control

The sensor core of the MT9V124 is a progressive-scan

sensor that generates a stream of pixel data at a constant

frame rate. Figure 4 shows a block diagram of the sensor

core. It includes the VGA active-pixel array. The timing and

control circuitry sequences through the rows of the array,

resetting and then reading each row in turn. In the time

interval between resetting a row and reading that row, the

pixels in the row integrate incident light. The exposure is

controlled by varying the time interval between reset and

readout. Once a row has been selected, the data from each

column is sequenced through an analog signal chain,

including offset correction, gain adjustment, and ADC. The

final stage of sensor core converts the output of the ADC into

10-bit data for each pixel in the array.

The pixel array contains optically active and

light-shielded (dark) pixels. The dark pixels are used to

provide data for the offset-correction algorithms (black level

control).

The sensor core contains a set of control and status

registers that can be used to control many aspects of the

sensor behavior including the frame size, exposure, and gain

setting. These registers are controlled by the MCU firmware

and are also accessible by the host processor through the

two-wire serial interface.

The output from the sensor core is a Bayer pattern;

alternate rows are a sequence of either green and red pixels

or blue and green pixels. The offset and gain stages of the

analog signal chain provide per-color control of the pixel

data.

Figure 4. Sensor Core Block Diagram

Sensor Core

Control Registers System Control

10−Bit

Data Out

G1/G2

R/B

G1/G2

R/B

VGA

Active−Pixel

Sensor (APS)

Array

Analog

Processing ADC Digital

Processing

Timing

and

Control

Green1/Green2

Channel

Red/Blue

Channel

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The sensor core uses a Bayer color pattern, as shown in

Figure 5. The even-numbered rows contain green and red

pixels; odd-numbered rows contain blue and green pixels.

Even-numbered columns contain green and blue pixels;

odd-numbered columns contain red and green pixels.

Figure 5. Pixel Color Pattern Detail

Column readout direction

Row readout

direction

Black pixels

First clear

pixel

The MT9V124 sensor core pixel array is shown with pixel

(0,0) in the bottom right corner, which reflects the actual

layout of the array on the die. Figure 6 shows the image

shown in the sensor during normal operation.

When the image is read out of the sensor, it is read one row

at a time, with the rows and columns sequenced.

Figure 6. Imaging a Scene

Lens

Pixel (0,0)

Row

Readout

Order

Column Readout Order

Scene

Sensor (rear view)

The sensor core supports different readout options to

modify the image before it is sent to the IFP. The readout can

be limited to a specific window size of the original pixel

array.

By changing the readout order, the image can be mirrored

in the horizontal direction.

The image output size is set by programming row and

column start and end address registers. The edge pixels in the

648 ×488 array are present to avoid edge effects and should

not be included in the visible window.

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When the sensor is configured to mirror the image

horizontally, the order of pixel readout within a row is

reversed, so that readout starts from the last column address

and ends at the first column address. Figure 7 shows a

sequence of 6 pixels being read out with normal readout and

reverse readout. This change in sensor core output is

corrected by the IFP.

Figure 7. Six Pixels in Normal and Column Mirror Readout Mode

(Internal Data Format before Serializer)

DOUT [9:0]

LINE_VALID

Normal readout

(9:0)

Reverse readout

(9:0)

DOUT[9:0]

Figure 8. Eight Pixels in Normal and Column Skip 2X Readout Mode

(Internal Data Format before Serializer)

DOUT[9:0]

LINE_VALID

Normal readout

(9:0)

DOUT[9:0]

LINE_VALID

Column skip readout

(9:0)

Figure 9 through Figure 11 show the different skipping

modes supported in MT9V124.

Figure 9. Pixel Readout (no skipping)

X incrementing

Y incrementing

Figure 10. Pixel Readout

(x_odd_inc = 3, y_odd_inc = 1)

X incrementing

Y incrementing

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Image Flow Processor

Image control processing in the MT9V124 is

implemented in the IFP hardware logic. The IFP registers

can be programmed by the host processor. For normal

operation, the microcontroller automatically adjusts the

operational parameters of the IFP. Figure 11 shows the

image data processing flow within the IFP.

VGA

Pixel Array

ADC

Raw Data

RAW 10

Digital

Gain

Control,

Shading

Correction

Defect Correction,

Nosie Reduction,

Color Interpolation,

IFP

Color Correction

Aperture

Correction

Gamma

Correction

(10−to−8 Lookup)

Statistics

Engine

Color Kill

Scaler

Output

Formatting

YUV to RGB

10/12−Bit

RGB

8−bit

RGB

8-bit

YUV

RGB to YUV

FIFO

LVDS Output

Output

Interface

Serializer

Test Pattern

Hue Rotate

Figure 11. Image Flow Processor

MUX

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For normal operation of the MT9V124, streams of raw

image data from the sensor core are continuously fed into the

color pipeline. The MT9V124 features an automatic color

bar test pattern generation function to emulate sensor images

as shown in Figure 12.

Color bar test pattern generation can be selected by

programming a register.

Figure 12. Color Bar Test Pattern

Test Pattern Example

REG= 0x8400, 0x15 // SEQ_CMD

REG= 0x8400, 0x16 // SEQ_CMD

REG= 0x8400, 0x17 // SEQ_CMD

REG= 0x8400, 0x18 // SEQ_CMD

REG= 0x8400, 0x19 // SEQ_CMD

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Image Corrections

Image stream processing starts with multiplication of all

pixel values by a programmable digital gain. This can be

independently set to separate values for each color channel

(R, Gr, Gb, B). Independent color channel digital gain can

be adjusted with variables.

Lenses tend to produce images whose brightness is

significantly attenuated near the edges. There are also other

factors causing fixed pattern signal gradients in images

captured by image sensors. The cumulative result of all these

factors is known as image shading. The MT9V124 has an

embedded shading correction module that can be

programmed to counter the shading effects on each

individual R, Gb, Gr, and B color signal.

The IFP performs continuous defect correction that can

mask pixel array defects such as high dark-current (hot)

pixels and pixels that are darker or brighter than their

neighbors due to photoresponse nonuniformity. The module

is edge-aware with exposure that is based on configurable

thresholds. The thresholds are changed continuously based

on the brightness of the current scene. Enabling and

disabling noise reduction, and setting thresholds can be

defined through variable settings.

Color Interpolation and Edge Detection

In the raw data stream fed by the sensor core to the IFP,

each pixel is represented by a 10-bit integer, which can be

considered proportional to the pixel’s response to a

one-color light stimulus, red, green, or blue, depending on

the pixel’s position under the color filter array. Initial data

processing steps, up to and including the defect correction,

preserve the one-color-per-pixel nature of the data stream,

but after the defect correction it must be converted to a

three-colors-per-pixel stream appropriate for standard color

processing. The conversion is done by an edge-sensitive

color interpolation module. The module adds the incomplete

color information available for each pixel with information

extracted from an appropriate set of neighboring pixels. The

algorithm used to select this set and extract the information

seeks the best compromise between preserving edges and

filtering out high-frequency noise in flat field areas. The

edge threshold can be set through variable settings.

Color Correction and Aperture Correction

To achieve good color fidelity of the IFP output,

interpolated RGB values of all pixels are subjected to color

correction. The IFP multiplies each vector of three pixel

colors by a 3 ×3 color correction matrix. The color

correction matrix can either be programmed by the user or

automatically selected by the AWB algorithm implemented

in the IFP. Color correction should ideally produce output

colors that are independent of the spectral sensitivity and

color crosstalk characteristics of the image sensor. The

optimal values of the color correction matrix elements

depend on those sensor characteristics. The color correction

variables can be adjusted through variable settings.

To increase image sharpness, a programmable 2D

aperture correction (sharpening filter) is applied to

color-corrected image data. The gain and threshold for 2D

correction can be defined through variable settings.

Gamma Correction

The gamma correction curve (as shown in Figure 13) is

implemented as a piecewise linear function with 19 knee

points, taking 12-bit arguments and mapping them to 8-bit

output. The abscissas of the knee points are fixed at 0, 64,

128, 256, 512, 768, 1024, 1280, 1536, 1792, 2048, 2304,

2560, 2816, 3072, 3328, 3584, 3840, and 4096.

The MT9V124 IFP includes a block for gamma correction

that has the capability to adjust its shape, based on

brightness, to enhance the performance under certain

lighting conditions. Two custom gamma correction tables

may be uploaded, one corresponding to a brighter lighting

condition, the other one corresponding to a darker lighting

condition. The final gamma correction table used depends

on the brightness of the scene and can take the form of either

uploaded tables or an interpolated version of the two tables.

A single (non-adjusting) table for all conditions can also be

used.

Figure 13. Gamma Correction Curve

amma

orrection

100

150

200

250

300

0 1000 2000 3000 4000

Input RGB, 12−bit

Output RGB, 8−bit

0.45

Special effects like negative image, sepia, or B/W can be

applied to the data stream at this point. These effects can be

enabled and selected by registers.

To remove high- or low-light color artifacts, a color kill

circuit is included. It affects only pixels whose luminance

exceeds a certain preprogrammed threshold. The U and V

values of those pixels are attenuated proportionally to the

difference between their luminance and the threshold.

Image Scaling and Cropping

To ensure that the size of images output by the MT9V124

can be tailored to the needs of all users, the IFP includes a

scaler module. When enabled, this module performs

rescaling of incoming images-shrinks them to selected

width and height without reducing the field of view and

without discarding any pixel values. The scaler ratios are

computed from image output size and the FOV. The scaled

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output must not be greater than 352. Output widths greater

than this must not use the scaler.

By configuring the cropped and output windows to

various sizes, different zooming levels for 4X, 2X, and 1X

can be achieved. The height and width definitions for the

output window must be equal to or smaller than the cropped

image. The image cropping and scaler module can be used

together to implement a digital zoom.

Hue Rotate

The MT9V124 has integrated hue rotate. This feature will

help for improving the color image quality and give

customers the flexibility for fine color adjustment and

special color effects.

Figure 14. 05 Hue

REG= 0xA00F, 0x00 // CAM_HUE_ANGLE

Figure 15. −225 Hue

REG= 0xA00F, 0xEA // CAM_HUE_ANGLE

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Figure 16. +225 Hue

REG= 0xA00F, 0x16 // CAM_HUE_ANGLE

Auto Exposure

The AE algorithm performs automatic adjustments of the

image brightness by controlling exposure time, and analog

gains of the sensor core as well as digital gains applied to the

image.

The AE algorithm analyzes image statistics collected by

the exposure measurement engine, and then programs the

sensor core and color pipeline to achieve the desired

exposure. AE uses 4 × 4 exposure statistics windows, which

can be scaled in size to cover any portion of the image.

The MT9V124 uses Average Brightness Tracking

(Average Y), which uses a constant average tracking

algorithm where a target brightness value is compared to a

current brightness value, and the gain and integration time

are adjusted accordingly to meet the target requirement. The

MT9V124 also has a weighted AE algorithm that allows the

sensor to be configured to respond to scene illuminance

based on each of the weights in the windows.

The auto exposure can be configured to respond to scene

illuminance based on certain criteria by adjusting gains and

integration time based on scene brightness.

Auto White Balance

The MT9V124 has a built-in AWB algorithm designed to

compensate for the effects of changing spectra of the scene

illumination on the quality of the color rendition. The

algorithm consists of two major parts: a measurement

engine performing statistical analysis of the image and a

module performing the selection of the optimal color

correction matrix, digital, and sensor core analog gains.

While default settings of these algorithms are adequate in

most situations, the user can reprogram base color correction

matrices and place limits on color channel gains.

The AWB algorithm estimates the dominant color

temperature of a light source in a scene and adjusts the B/G,

R/G gain ratios accordingly to produce an image for sRGB

display in which grey and white surfaces are reproduced

faithfully. This usually means that R,G,B are roughly equal

for these surfaces hence the word “balance”.

The AWB algorithm uses statistics collected from the last

frame to calculate the required B/G and R/G ratios and set

the blue and red analog sensor gains and digital SOC gains

to reproduce the most accurate grey and white surfaces

Flicker Detection and Avoidance

Flicker occurs when the integration time is not an integer

multiple of the period of the light intensity. The automatic

flicker detection module does not compensate for the flicker,

but rather avoids it by detecting the flicker frequency and

adjusting the integration time. For integration times below

the light intensity period (10 ms for 50 Hz environment,

8.33 ms for 60 Hz environment), flicker cannot be avoided.

While this fast flickering is marginally detectable by the

human eye, it is very noticeable in digital images because the

flicker period of the light source is very close to the range of

digital images’ exposure times.

Many CMOS sensors use a “rolling shutter” readout

mechanism that greatly improves sensor data readout times.

This allows pixel data to be read out much sooner than other

methods that wait until the entire exposure is complete

before reading out the first pixel data. The rolling shutter

mechanism exposes a range of pixel rows at a time. This

range of exposed pixels starts at the top of the image and then

“rolls” down to the bottom during the exposure period of the

frame. As each pixel row completes its exposure, it is ready

to be read out. If the light source oscillates (flickers) during

this rolling shutter exposure period, the image appears to

have alternating light and dark horizontal bands.

If the sensor uses the traditional snapshot readout

mechanism, in which all pixels are exposed at the same time

and then the pixel data is read out, then the image may appear

overexposed or underexposed due to light fluctuations from

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the flickering light source. Lights operating on AC electric

systems produce light flickering at a frequency of 100 Hz or

120 Hz, twice the frequency of the power line.

To avoid this flicker effect, the exposure times must be

multiples of the light source flicker periods. For example, in

a scene lit by 120 Hz lighting, the available exposure times

are 8.33 ms, 16.67 ms, 25 ms, 33.33 ms, and so on. (The need

for an exposure time less than 8.33 ms under artificial light

is extremely rare.)

In this case, the AE algorithm must limit the integration

time to an integer multiple of the light’s flicker period.

By default, the MT9V124 does all of this automatically,

ensuring that all exposure times avoid any noticeable light

flicker in the scene. The MT9V124 AE algorithm is always

setting exposure times to be integer multipliers of either 100

Hz or 120 Hz. The flicker detection module keeps

monitoring the incoming frames to detect whether the

scene’s lighting has changed to the other of the two light

source frequencies. A 50 Hz/60 Hz Tungsten lamp can be

used to calibrate the flicker detect settings.

Output Conversion and Formatting

The YUV data stream can either exit the color pipeline as

is or be converted before exit to an alternative YUV or RGB

data format.

Color Conversion Formulas

Y’U’V’:

This conversion is BT 601 scaled to make YUV range

from 0 through 255. This setting is recommended for JPEG

encoding and is the most popular, although it is not well

defined and often misused in various operating systems.

YȀ+0.299 RȀ)0.587 GȀ)0.114 BȀ(eq. 1)

UȀ+0.564 (BȀ*YȀ))128 (eq. 2)

VȀ+0.713 (RȀ*YȀ))128 (eq. 3)

There is an option where 128 is not added to U’V’.

Y’Cb’Cr’ Using sRGB Formulas:

The MT9V124 implements the sRGB standard. This

option provides YCbCr coefficients for a correct 4:2:2

transmission.

NOTE: 16 < Y601< 235; 16 < Cb < 240; 16 < Cr < 240;

and 0 < = RGB < = 255

YȀ+(0.2126 RȀ)0.7152 GȀ)0.0722 BȀ)

(219ń256) )16 (eq. 4)

CbȀ+0.5389 (BȀ*YȀ) (224ń256) )128 (eq. 5)

CrȀ+0.635 (RȀ*YȀ) (224ń256) )128 (eq. 6)

Y’U’V’ Using sRGB Formulas:

These are similar to the previous set of formulas, but have

YUV spanning a range of 0 through 255.

YȀ+0.2126 RȀ)0.7152 GȀ)0.0722 BȀ) (eq. 7)

)128

UȀ+0.5389 (BȀ*YȀ))128 +

+*0.1146 RȀ*0.3854 GȀ)0.5 BȀ)128

(eq. 8)

VȀ+0.635 (RȀ*YȀ))128 +

+0.5 RȀ*0.4542 GȀ*0.0458 BȀ)128

(eq. 9)

There is an option to disable adding 128 to U’V’. The

reverse transform is as follows:

RȀ+Y)1.5748 (V *128) (eq. 10)

GȀ+Y*0.1873 (U *128) *0.4681 (V *128) (eq. 11)

BȀ+Y)1.8556 (U *128) (eq. 12)

Uncompressed YUV/RGB Data Ordering

The MT9V124 supports swapping YCbCr mode, as

illustrated in Table 5.

Table 5. YCbCr OUTPUT DATA ORDERING

Mode Data Sequence

Default (no Swap) CbiYiCriYi+1

Swapped CrCb CriYiCbiYi+1

Swapped YC YiCbiYi+1 Cri

Swapped CrCb, YC YiCriYi+1 Cbi

The RGB output data ordering in default mode is shown

in Table 6. The odd and even bytes are swapped when

luma/chroma swap is enabled. R and B channels are bitwise

swapped when chroma swap is enabled.

Table 6. RGB ORDERING IN DEFAULT MODE

Mode (Swap Disabled) Byte D7D6D5D4D3D2D1D0

565RGB Odd R7R6R5R4R3G7G6G5

Even G4G3G2B7B6B5B4B3

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Uncompressed 10-Bit Bypass Output

Raw 10-bit Bayer data from the sensor core can be output

in bypass mode by using DOUT[7:0] with a special 8 + 2 data

format, shown in Table 7.

Table 7. 2-BYTE BAYER FORMAT

Byte Bits Used Bit Sequence

Odd Bytes 8 Data Bits D9D8D7D6D5D4D3D2

Even Bytes 2 Data Bits + 6 Unused Bits 0 0 0 0 0 0 D1D0

BT656

YUV data can also be output in BT656 format with only

Odd field SAV/EAV codes. The BT656 data output will be

progressive data and not interlaced (R0x3C00[5] = 1).

Figure 17 depicts the data format before the serializer

internal to the device, or after the external deserializer.

Active Video

80 80 80 80 80 80 80 80 80 80 80 10101010101010 00 00 00 00 00Cb Y Cr Y Y Cr YCb FF B6FF00 00 9DFF Y Cr YCb Cr YCb Y FF

Data[7:0]

Figure 17. BT656 Image Data with Odd SAV/EAV Codes

10 10 10 00 80

Blanking SAV

H Blank Image

EAV Blanking

H Blank

SAV Image EAV Blanking

H Blank

To change internal registers and RAM variables of

MT9V124, use the two-wire serial interface through the

external host device.

The sequencer is responsible for coordinating all events

triggered by the user.

The sequencer provides the high-level control of the

MT9V124. Commands are written to the command variable

to start streaming, stop streaming, and to select test pattern

modes. Command execution is confirmed by reading back

the command variable with a value of zero. The sequencer

state variable can also be checked for transition to the

desired state. All configuration of the sensor (start/stop

row/column, mirror, skipping) and the SOC (image size,

format) and automatic algorithms for AE, AWB, low light,

are performed when the sequencer is in the stopped state.

When the sequencer is in the idle or test pattern state the

algorithms and register updates are not performed, allowing

the host complete manual control

Table 8. SUMMARY OF MT9V124 VARIABLES

Name Variable Description

Monitor Variables General Information

Sequencer Variables Programming Control Interface

FD Variables Flicker Detect

AE_Track Variables Auto Exposure

AWB Variables Auto White Balance

Stat Variables Statistics

Low Light Variables Low Light

Cam Variables Sensor Specific Settings

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SERIAL LOW VOLTAGE DIFFERENTIAL SIGNALING (LVDS) OUTPUT

The MT9V124 provides a serial high-speed output port

which supports all the data formats. MT9V124 is intended

to drive standard IEEE 1596.3−1996 LVDS

receiver/deserializers. The internal serializer transforms the

parallel data into serial in a 12-bit packet, allowing the data

be transported via a lengthy (several meters) twisted pair

cable.

The LVDS output requires a differential termination

resistor (Rtx_term = 140 Ω ±1%) that must be provided

off-chip and close to the LVDS pins.

Figure 18. LVDS Typical Serial Interface

100 Ω

140 Ω±1%

100 Ω twisted-pair

LVDS

DRIVER

LVDS

RECEIVER

LVDS Data Packet Format

The LVDS output is the standard 12-bit package with start

bit, 10-bit payload and stop bit supported by many off the

shelf deserializers.

Table 9 describes the LVDS packet format; Figure 19

shows the LVDS data timing.

Table 9. LVDS PACKET FORMAT

12-Bit Packet Data Format

Bit[0] START BIT “1”

Bit[1] PixelData[0]

Bit[2] PixelData[1]

Bit[3] PixelData[2]

Bit[4] PixelData[3]

Bit[5] PixelData[4]

Bit[6] PixelData[5]

Bit[7] PixelData[6]

Bit[8] PixelData[7]

Bit[9] LINEVALID (LV)

Bit[10] FRAMEVALID (FV)

Bit[11] STOP BIT “0”

Figure 19. LVDS Serial Output Timing

D0 D1 D2 D3 D4 D5 D6 D7 LV FV

tDW

Internal Shift Clock

LVDS Serial Out STOP

(0)

START

(0)

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Table 10. LVDS SERIAL OUTPUT DATA TIMING (FOR EXTCLK = 22 MHz)

Name Min Typical Max Unit

tDW 3.78 3.78 4.629 nS

1/tDW 216 264 264 Mbps

Table 11. EXTCLK INPUT RANGE

Name Min Typical Max Unit

EXTCLK 18 22 44 MHz

If EXTCLK is greater than 22 MHz, the PLL must be set

to obtain an equivalent internal pixel clock to 22 MHz. The

internal pixel clock is multiplied by 12 to achieve the

serializer output frequency of maximum 264 MHz.

TWO-WIRE SERIAL INTERFACE

The two-wire serial interface bus enables read and write

access to control and status registers within the MT9V124.

The interface protocol uses a master/slave model in which

a master controls one or more slave devices. The MT9V124

always operates in slave mode. The host (master) generates

a clock (SCLK) that is an input to the MT9V124 and is used

to synchronize transfers. Data is transferred between the

master and the slave on a bidirectional signal (SDATA).

Protocol

Data transfers on the two-wire serial interface bus are

performed by a sequence of low-level protocol elements, as

follows:

1. a (repeated) start condition

2. a slave address/data direction byte

3. a 16-bit register address

(8-bit addresses are not supported)

4. an (a no) acknowledge bit

5. a 16-bit data transfer

(8-bit data transfers are supported using XDMA

byte access)

6. a stop condition

The bus is idle when both SCLK and SDATA are HIGH.

Control of the bus is initiated with a start condition, and the

bus is released with a stop condition. Only the master can

generate the start and stop conditions.

A start condition is defined as a HIGH-to-LOW transition

on SDATA while SCLK is HIGH.

At the end of a transfer, the master can generate a start

condition without previously generating a stop condition;

this is known as a repeated start or restart condition.

A stop condition is defined as a LOW-to-HIGH transition

on SDATA while SCLK is HIGH.

Data is transferred serially, 8 bits at a time, with the most

significant bit (MSB) transmitted first. Each byte of data is

followed by an acknowledge bit or a no-acknowledge bit.

This data transfer mechanism is used for the slave

address/data direction byte and for message bytes. One data

bit is transferred during each SCLK clock period. SDATA can

change when SCLK is LOW and must be stable while SCLK

is HIGH.

MT9V124 Slave Address

Bits [7:1] of this byte represent the device slave address

and bit [0] indicates the data transfer direction. A “0” in bit

[0] indicates a WRITE, and a “1” indicates a READ. The

slave address default is 0x7A.

Messages

Message bytes are used for sending MT9V124 internal

16-bit address (two bytes) and 16-bit data to access internal

registers. Refer to READ and WRITE cycles in Figure 20

through Figure 24.

Each 8-bit data transfer is followed by an acknowledge bit

or a no-acknowledge bit in the SCLK clock period following

the data transfer. The transmitter (which is the master when

writing, or the slave when reading) releases SDATA. The

receiver indicates an acknowledge bit by driving SDATA

LOW. For data transfers, SDATA can change when SCLK is

LOW and must be stable while SCLK is HIGH.

The no-acknowledge bit is generated when the receiver

does not drive SDATA low during the SCLK clock period

following a data transfer. A no-acknowledge bit is used to

terminate a read sequence.

Typical Operation

A typical READ or WRITE sequence begins by the

master generating a start condition on the bus. After the start

condition, the master sends the 8-bit slave address/data

direction byte. The last bit indicates whether the request is

for a READ or a WRITE, where a “0” indicates a WRITE

and a “1” indicates a READ. If the address matches the

address of the slave device, the slave device acknowledges

receipt of the address by generating an acknowledge bit on

the bus.

If the request was a WRITE, the master then transfers the

16-bit register address to which a WRITE will take place.

This transfer takes place as two 8-bit sequences and the slave

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sends an acknowledge bit after each sequence to indicate

that the byte has been received. The master will then transfer

the 16-bit data, as two 8-bit sequences and the slave sends an

acknowledge bit after each sequence to indicate that the byte

has been received. The master stops writing by generating

a (re)start or stop condition. If the request was a READ, the

master sends the 8-bit write slave address/data direction byte

and 16-bit register address, just as in the WRITE request.

The master then generates a (re)start condition and the 8-bit

read slave address/data direction byte, and clocks out the

acknowledge bit after each 8-bit transfer. The data transfer

is stopped when the master sends a no-acknowledge bit.

Single READ from Random Location

Figure 20 shows the typical READ cycle of the host to

MT9V124. The first 2 bytes sent by the host are an internal

16-bit register address. The following 2-byte READ cycle

sends the contents of the registers to host.

Figure 20. Single READ from Random Location

Previous Reg Address, N Reg Address, M M+1

S0 1 PA

Slave

Address

Reg

Address[15:8]

Reg

Address[7:0] Slave Address

S = Start Condition

P = Stop Condition

Sr = Restart Condition

A = Acknowledge

A = No-acknowledge

Slave to Master

Master to Slave

A A A A Read Data

Single READ from Current Location

Figure 21 shows the single READ cycle without writing

the address. The internal address will use the previous

address value written to the register.

Figure 21. Single Read from Current Location

N+LN+L−1N+2N+1Previous Reg Address, N

PAS 1 Read DataASlave Address Read DataRead Data Read DataAAA

Sequential READ, Start from Random Location

This sequence (Figure 22) starts in the same way as the

single READ from random location (Figure 20). Instead of

generating a no-acknowledge bit after the first byte of data

has been transferred, the master generates an acknowledge

bit and continues to perform byte READs until “L” bytes

have been read.

Figure 22. Sequential READ, Start from Random Location

Previous Reg Address, N Reg Address, M

S0Slave Address A AReg Address[15:8]

M+1

A A A1SrReg Address[7:0] Read DataSlave Address

M+LM+L−1M+L−2M+1 M+2 M+3

ARead Data A Read Data ARead Data Read Data

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Sequential READ, Start from Current Location

This sequence (Figure 23) starts in the same way as the

single READ from current location (Figure 21). Instead of

generating a no-acknowledge bit after the first byte of data

has been transferred, the master generates an acknowledge

bit and continues to perform byte reads until “L” bytes have

been read.

Figure 23. Sequential READ, Start from Current Location

N+LN+L−1N+2N+1Previous Reg Address, N

SAS 1 Read DataASlave Address Read DataRead Data Read DataAAA

Single Write to Random Location

Figure 24 shows the typical WRITE cycle from the host

to the MT9V124. The first 2 bytes indicate a 16-bit address

of the internal registers with most-significant byte first. The

following 2 bytes indicate the 16-bit data.

Figure 24. Single WRITE to Random Location

Previous Reg Address, N Reg Address, M M+1

S0 PSlave Address Reg Address[15:8] Reg Address[7:0] A

A A Write Data

Sequential WRITE, Start at Random Location

This sequence (Figure 25) starts in the same way as the

single WRITE to random location (Figure 24). Instead of

generating a no-acknowledge bit after the first byte of data

has been transferred, the master generates an acknowledge

bit and continues to perform byte writes until “L” bytes have

been written. The WRITE is terminated by the master

generating a stop condition.

Figure 25. Sequential WRITE, Start at Random Location

Previous Reg Address, N Reg Address, M M+1

S0Slave Address A Reg Address[15:8] A A AReg Address[7:0]

M+LM+L−1M+L−2M+1 M+2 M+3

Write Data AA AS

Write Data

AWrite Data Write Data

One-Time Programming Memory (OTPM)

The MT9V124 has one-time programmable memory

(OTPM) for supporting defect correction, module ID, and

other customer-related information. There are 2784 bits of

OTPM available for features such as Lens Shading

Correction, Color Correction Matrix, White Balance

Weight, and user-defined information. The OTPM

programming requires the data to be first placed in OTPM

buffer and the presence of VPP. The proper procedure and

timing must be followed.

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SPECTRAL CHARACTERISTICS

CRA vs. Image Height Plot

Image Height CRA

(deg)

(%) (mm)

10 20 30 40 50 60 70 80 90 100 110

Figure 26. Chief Ray Angle (CRA) vs. Image Height

CRA (deg)

Image Height (%)

0 0 0

5 0.035 1.23

10 0.070 2.46

15 0.105 3.70

20 0.140 4.94

25 0.175 6.18

30 0.210 7.43

35 0.245 8.67

40 0.280 9.90

45 0.315 11.13

50 0.350 12.36

55 0.385 13.57

60 0.420 14.77

65 0.455 15.97

70 0.490 17.14

75 0.525 18.31

80 0.560 19.45

85 0.595 20.58

90 0.630 21.69

95 0.665 22.77

100 0.700 23.83

Figure 27. Quantum Efficiency

350 400 450 500 550 600 650 700 750

Wavelength (nm)

Quantum Efficiency (%)

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ELECTRICAL SPECIFICATIONS

Table 12. ABSOLUTE MAXIMUM RATINGS

Symbol Parameter

Rating

Unit

Min Max

VDD Core Digital Voltage –0.3 2.4 V

VDD_IO I/O Digital Voltage –0.3 4.0 V

VAA Analog Voltage –0.3 4.0 V

VAA_PIX Pixel Supply Voltage –0.3 4.0 V

VPP OTPM Power Supply 7.5 9.5 V

VIN Input Voltage –0.3 VDD_IO + 0.3 V

TOP Operating Temperature (Measure at Junction) –30 70 °C

TSTG (Note 1) Storage Temperature –40 85 °C

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. This is a stress rating only, and functional operation of the device at these or any other conditions above those indicated in the product

specification is not implied. Exposure to absolute maximum rating conditions for extended periods may affect device reliability.

Recommended Operating Conditions

Table 13. OPERATING CONDITIONS

Symbol Parameter Min Typ Max Units

VDD Core Digital Voltage 1.7 1.8 1.95 V

VDD_IO I/O Digital Voltage 2.5 2.8 3.1 V

1.7 1.8 1.95 V

VAA Analog Voltage 2.5 2.8 3.1 V

VAA_PIX Pixel Supply Voltage 2.5 2.8 3.1 V

VDD_PLL PLL Supply Voltage 2.5 2.8 3.1 V

VPP OTPM Power Supply 8.5 8.5 9 V

TJOperating Temperature (at Junction) –30 55 70 °C

Table 14. DC ELECTRICAL CHARACTERISTICS

Symbol Parameter Condition Min Max Unit

VIH Input HIGH Voltage 0.7 * VDD_IO VDD_IO + 0.5 V

VIL Input LOW Voltage –0.3 0.3 * VDD_IO V

IIN Input Leakage Current VIN = 0V or VIN = VDD_IO 10 μA

VOH Output HIGH Voltage VDD_IO = 1.8 V, IOH = 2 mA 1.7 – V

VDD_IO = 1.8 V, IOH = 4 mA 1.6 – V

VDD_IO = 1.8 V, IOH = 8 mA 1.4 – V

VDD_IO = 2.8 V, IOH = 2 mA 2.7 – V

VDD_IO = 2.8 V, IOH = 4 mA 2.6 – V

VDD_IO = 2.8 V, IOH = 8 mA 2.5 – V

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Table 14. DC ELECTRICAL CHARACTERISTICS (continued)

Symbol UnitMaxMinConditionParameter

VOL Output LOW Voltage VDD_IO = 1.8 V, IOH = 2 mA – 0.1 V

VDD_IO = 1.8 V, IOH = 4 mA – 0.2 V

VDD_IO = 1.8 V, IOH = 8 mA – 0.4 V

VDD_IO = 2.8 V, IOH = 2 mA – 0.1 V

VDD_IO = 2.8 V, IOH = 4 mA – 0.2 V

VDD_IO = 2.8 V, IOH = 8 mA – 0.4 V

Table 15. OPERATING/STANDBY CURRENT CONSUMPTION

(fEXTCLK = 44 MHz; voltages = Typ or Max; TJ = Typ or Max; excludes VDD_IO current)

Symbol Parameter Condition Typ Unit

IDD Digital Operating Current 9.5 mA

IAA Analog Operating Current 7 mA

IDD_PLL PLL Supply Current 5 mA

Total Supply Current 21.5 mA

Total Power Consumption 55 mW

Hard Standby Total Standby Current when Asserting the

STANDBY Signal

19 μA

Standby Power 44 μW

Soft Standby

(Clock On)

Total Standby Current fEXTCLK = 44 MHz,

Soft standby mode

1.67 mA

Standby Power 3.016 mW

Soft Standby

(Clock Off)

Total Standby Current Soft Standby Mode 19 μA

Standby Power 44.2 μW

Table 16. LVDS OUTPUT PORT DC SPECIFICATIONS

Parameter Symbol Conditions Min Typ Max Units

Output Voltage High Voh 1650 mV

Output Voltage Low Vol 850 mV

Differential Output Voltage Vod 280 360 460 mV

Output Offset Voltage Vos See text 1000 1192 1400 mV

Single-ended Output Resistance Ro 150 250 Ω

Output Resistance Mismatch ΔRo 12 %

Reflection Coefficient Mismatch Δρ 8 %

Differential Output Mismatch ΔVod 6 mV

Offset Voltage Mismatch ΔVos See text 30 mV

Output Short-circuit Current Isa, Isb 17 mA

Output Short-circuit Current Isab 10 mA

Standing Power-supply Current Ivddio 8 mA

Clock Signal Duty Cycle clock 250 MHz;

Cload = 6pF

48 53 5

Differential Signal Rise Time trCload = 6pF 360 ps

Differential Signal Fall Time tfCload = 6pF 360 ps

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Table 16. LVDS OUTPUT PORT DC SPECIFICATIONS (continued)

UnitsMaxTypMinConditionsSymbolParameter

Propagation Delay tpCload = 6pF 2.5 ns

Differential Skew tskew Cload = 6pF πΩ

Table 17. TWO-WIRE SERIAL INTERFACE TIMING DATA

(fEXTCLK = 22 MHz; VDD = 1.8 V; VDD_IO = 1.8 V; VAA = 2.8 V; VAA_PIX = 2.8 V; VDD_PLL = 2.8 V)

Parameter Symbol

Standard-Mode Fast-Mode

Unit

Min Max Min Max

SCLK Clock Frequency fSCL 0 100 0 400 KHz

Hold Time (repeated) START Condition.

After this Period, the First Clock Pulse is Generated tHD;STA 4.0 −0.6 −μS

LOW Period of the SCLK Clock tLOW 4.7 −1.3 −μS

HIGH Period of the SCLK Clock tHIGH 4.0 −0.6 −μS

Set-up Time for a Repeated START Condition tSU;STA 4.7 −0.6 −μS

Data Hold Time tHD;DAT 0

(Note 4)

3.45

(Note 5)

(Note 6)

0.9

(Note 5)

μS

Data Set-up Time tSU;DAT 250 −100 (Note 6) −nS

Rise Time of Both SDATA and SCLK Signals tr−1000 20 + 0.1Cb

(Note 7)

300 nS

Fall Time of Both SDATA and SCLK Signals tf−300 20 + 0.1Cb

(Note 7)

300 nS

Set-up Time for STOP Condition tSU;STO 4.0 −0.6 −μS

Bus Free Time between a STOP and START Condition tBUF 4.7 −1.3 −μS

Capacitive Load for Each Bus Line Cb −400 −400 pF

Serial Interface Input Pin Capacitance CIN_SI −3.3 −3.3 pF

SDATA Max Load Capacitance CLOAD_SD −30 −30 pF

SDATA Pull-up Resistor RSD 1.5 4.7 1.5 4.7 KΩ

1. This table is based on I2C standard (v2.1 January 2000). On Semiconductor

2. Two-wire control is I2C−compatible

3. All values referred to VIHmin = 0.9 VDD and VILmax = 0.1VDD levels. Sensor EXCLK = 22 MHz

4. A device must internally provide a hold time of at least 300 ns for the SDATA signal to bridge the undefined region of the falling edge of SCLK.

5. The maximum tHD;DAT has only to be met if the device does not stretch the LOW period (tLOW) of the SCLK signal

6. A Fast-mode I2C-bus device can be used in a Standard-mode I2C-bus system, but the requirement tSU;DAT 250 ns must then be met. This

will automatically be the case if the device does not stretch the LOW period of the SCLK signal. If such a device does stretch the LOW period

of the SCLK signal, it must output the next data bit to the SDATA line tr max + tSU;DAT = 1000 + 250 = 1250 ns (according to the Standard-mode

I2C-bus specification) before the SCLK line is released

7. Cb = total capacitance of one bus line in pF

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Figure 28. Two-Wire Serial Bus Timing Parameters

SCLK

SDATA

SCLK

SDATA

Write Start Ack

Read Start Ack

tSHAR tAHSR tSDHR

tSDSR

Read Sequence

Write Sequence

Read

Address

Bit 7

Read

Address

Bit 0

Value

Bit 7

Value

Bit 0

Write

Address

Bit 7

Write

Address

Bit 0

Value

Bit 7

Value

Bit 0

tSRTS

tSCLK tSDH

tSDS tSHAW

Stop

AHSW

STPS

tSRTH

Ack

STPH

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POWER SEQUENCE

Powering up the sensor requires the supply rails to be

applied in a particular order to ensure sensor start up in a

normal operation and prevent undesired condition such as

latch up from happening. Refer to Figure 29 and Table 18

for detailed timing requirement.

Figure 29. Power-Up Sequence

AA , VDD_IO, VDD_PHY

VDD

EXTCLK t2

Internal POR

SCLK

SDATA

Table 18. POWER UP SIGNAL TIMING

Symbol Parameter Min Typ Max Unit

t1 Delay from VDD to VAA and VDD_IO 0 – 500 ms

t2 EXTCLK Activation t1 100 −ms

t3 Internal POR Duration 70 −– EXTCLKs

t4 First I2C Write 50 − − EXTCLKs

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ON Semiconductor and are registered trademarks of Semiconductor Components Industries, LLC (SCILLC). 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

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