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Friend,
I introduce you the measurable term called SNR = Signal-to-Noise Ratios, that is how sensor engineer/designer evaluate the QUALITY/EFFICIENCY of a sensor.
The references and detail complicated equations and formulas are left to the end.
為什麼 用DC 拍照的 noise 比數碼單鏡反光相機多?
DC = P&S camera, the sensor size is very small 1/1.6-1/1.8 inches, meaning the sensor manufacturer need to pack N megapixels in to a tiny area. each tiny cell need to process the signal received from more photons, the energy comsumption per cell is increased, and the temperature increased in proportion in that tiny area.
DSLR has a bigger sensor, more than 1-2 inch in size ..., therefore, DSLR allow longer exposure/BULB SHUTTER and higher ISO sensitivity, because of the bigger sensor, and the more advanced signal processing.
圖片參考:
http://www.dpreview.com/news/0209/canon/eos1ds/canonsensors-001.jpg
CMOS Sensor by Canon
圖片參考:
http://www.robgalbraith.com/data/1/rec_imgs/135_nikon_d2h_LBCAST.jpg
CCD sensor by Nikon
圖片參考:
http://learn.hamamatsu.com/articles/images/signaltonoisefigure1.jpg
SNR = Signal-to-Noise Ratios, the BIGGER THE NUMBER, the better sensor performance, or LESS NOISE.
Sensor noise
Noise is an unwanted signal, either contained in the relevant light
signal or added to it by the imaging process.
Noise prevents accurate measurement and
evaluation of the light signal distribution (image).
For any electronic measuring system, the signal-to-noise ratio (SNR) characterizes the quality of a measurement and determines the ultimate performance of the system.
The three(3) primary sources of noise in a CCD imaging system are photon noise, dark noise, and read noise, all of which must be considered in the SNR calculation.
1. Photon or shot noise
2. CCD/CMOS image sensor noise
3. Read out or amplifier noise
1. photon or shot noise
As a natural part of light, the number of photons impinging on a CCD/CMOS image
sensor that generates charge carriers is not exact, and can only be described
using probability. Photon or shot noise is a characteristic of light, which is best
described by a statistical distribution with an uncertainty. This noise is directly
proportional to the magnitude of the light signal itself.
(related to sensor size, the more photons collected in a fixed area, the more
photo noise.)
2. CCD/CMOS image sensor noise
Noise influences that may occur on a CCD/CMOS image sensor include:
- "dark charge" or "dark current" (e.g. thermally induced charge carriers)
Dark noise arises from statistical variation in the number of electrons thermally
generated within the silicon structure of the CCD,
which is independent of photon-induced signal, but highly dependent on device temperature.
The generation rate of thermal electrons at a given CCD temperature
is referred to as dark current.
Cooling the CCD reduces the dark current dramatically.
(related to the TEMPERATURE, the lower the power consumption, the less processing of photons in an area, the lower the temperature, the less noise.)
- transfer noise (additional or lost charge carriers due to shift of charge carriers
between the registers of a CCD/CMOS image sensor)
- fixed pattern noise (spatially fixed differences in noise behavior or sensitivity)
FIXED PATTERN (SPATIAL) NOISE
FPN refers to a non-temporal spatial noise and is due to device
mismatches in the pixels & color filters, variations in column
amplifiers, and mismatches between multiple PGAs and ADCs.
FPN can be either coherent or non-coherent.
- noise that is dependent on the setpoint of the CCD/CMOS image sensor, etc..
3. read out noise
A noise signal can be added during the conversion of the charge carriers into
a voltage signal and the subsequent processing and analog-to-digital conversion.
This is caused by the amplifier processing chain and the actual analog-to-digital
conversion process. This noise is uniformly added to the image.