Datasheet-1
Table Of Contents
- 1/3-Inch Wide-VGA CMOS Digital Image Sensor
- Features
- Applications
- Ordering Information
- Table of Contents
- List of Figures
- List of Tables
- General Description
- Ball Descriptions
- Pixel Data Format
- Color Device Limitations
- Output Data Format
- Serial Bus Description
- Two-Wire Serial Interface Sample Read and Write Sequences
- Feature Description
- Operational Modes
- Signal Path
- On-Chip Biases
- Window Control
- Blanking Control
- Pixel Integration Control
- Variable ADC Resolution
- Gain Settings
- Black Level Calibration
- Row-wise Noise Correction
- Automatic Gain Control and Automatic Exposure Control
- Pixel Clock Speed
- Hard Reset of Logic
- Soft Reset of Logic
- STANDBY Control
- Monitor Mode Control
- Read Mode Options
- LINE_VALID
- LVDS Serial (Stand-Alone/Stereo) Output
- LVDS Output Format
- Electrical Specifications
- Package Dimensions
- Appendix A – Serial Configurations
- Appendix B – Power-On Reset and Standby Timing
- Revision History
PDF: 3295348826/Source:7478516499 Aptina reserves the right to change products or specifications without notice.
MT9V022_DS - Rev.H 6/10 EN
44 ©2005 Aptina Imaging Corporation. All rights reserved.
MT9V022: 1/3-Inch Wide-VGA Digital Image Sensor
Electrical Specifications
Test 4: Dynamic Range
A temporal noise measurement is made with the image sensor in the dark and analog
gain changed to the maximum setting of 4X. Signals are measured in LSB on the sensor
output. Two consecutive dark frames are captured. Temporal noise is calculated as the
average pixel value of the difference frame:
(EQ 17)
Where S
1i
is the signal measured for the i-th pixel from the first frame, S
2i
is the signal
measured for the i-th pixel from the second frame, and N
p
is the total number of pix-
els contained in the array.
The dynamic range is calculated according to the following formula:
(EQ 18)
Where
σ
t
is the temporal noise measured in the dark at 4X gain.
Test 5: Signal-to-Noise Ratio
A flat-field light source (90 lux, color temperature 4400K, broadband, with IR cut filter) is
used as an illumination source. Signals are measured in LSB on the sensor output. Two
consecutive illuminated frames are captured. Temporal noise is calculated as the
average pixel value of the difference frame (according to the formula shown in Test 4).
The signal-to-noise ratio is calculated as the ratio of the average signal level to the
temporal noise according to the following formula:
(EQ 19)
Where σ
t
is the temporal noise measured from the illuminated frames, S
1i
is the signal
measured for the i-th pixel from the first frame, and N
p
is the total number of pixels
contained in the array.
σ
i
S
1i
S
2i
–()
2
i 1=
N
p
∑
2 N
p
⋅
------------------------------------=
DynamicRange 20
4 1022×
σ
t
---------------------
log⋅=
Signal to– Noise– Ratio–20
S
1i
i 1=
N
p
∑
⎝⎠
⎜⎟
⎜⎟
⎛⎞
N
p
⁄
⎝⎠
⎜⎟
⎜⎟
⎛⎞
σ
t
--------------------------------------
log⋅=










